VOLCANISM IN HAWAII Chapter 1
- .-...... ,. THE HAWAIIAN-EMPEROR VOLCANIC CHAIN Part I Geologic Evolution
By David A. Clague and G. Brent Dalrymple
ABSTRACT chain, the near-fixity of the hot spot, the chemistry and timing of The Hawaiian-Emperor volcanic chain stretches nearly the eruptions from individual volcanoes, and the detailed geom 6,000 km across the North Pacific Ocean and consists of at least etry of volcanism. None of the geophysical hypotheses pro t 07 individual volcanoes with a total volume of about 1 million posed to date are fully satisfactory. However, the existence of km3• The chain is age progressive with still-active volcanoes at the Hawaiian ewell suggests that hot spots are indeed hot. In the southeast end and 80-75-Ma volcanoes at the northwest addition, both geophysical and geochemical hypotheses suggest end. The bend between the Hawaiian and .Emperor Chains that primitive undegassed mantle material ascends beneath reflects a major change in Pacific plate motion at 43.1 ± 1.4 Ma Hawaii. Petrologic models suggest that this primitive material and probably was caused by collision of the Indian subcontinent reacts with the ocean lithosphere to produce the compositional into Eurasia and the resulting reorganization of oceanic spread range of Hawaiian lava. ing centers and initiation of subduction zones in the western Pacific. The volcanoes of the chain were erupted onto the floor of the Pacific Ocean without regard for the age or preexisting INTRODUCTION structure of the ocean crust. Hawaiian volcanoes erupt lava of distinct chemical com The Hawaiian Islands; the seamounts, hanks, and islands of positions during four major stages in their evolution and the Hawaiian Ridge; and the chain of Emperor Seamounts form an growth. The earliest stage is a submarine alkalic preahield array of shield volcanoes that stretches nearly 6,000 km across the stage, which is followed by the tholeiitic shield stage. The shield north Pacific Ocean (fig. 1.1). This unique geologic feature consists stage probably accounts for >95 percent of the volume of each volcano. The shield stage is followed by an alkalic postshield of more than 107 individual volcanoes with a combined volume 3 stage during which a thin cap of alkalic basalt and associated slightly greater than 1 million km (Bargar and Jackson, 1974). The differentiated lava covers the tholeiitic shield. After several chain is age progressive with still-active volcanoes at the southeast million years of erosion, alkalic rejuvenated-stage lava erupts end whereas those at the northwest end have ages of about 75-80 from isolated vents. An individual volcano may become extinct Ma. The volcanic ridge is surrounded by a symmetrical depression, before the sequence is complete. The alkalic preshield stage is only known from recent study of Loihi Seamount. Lava from the Hawaiian Deep, as much as 0.7 km deeper than the adjacent later eruptive stages has been identified from numerous sub ocean floor (Hamilton, 1957). The Hawaiian Deep is in turn merged volcanoes located west of the principal Hawaiian surrounded by the broad Hawaiian Arch. Islands. At the southeast end of the chain lie the eight principal Volcanic propagation rates along the chain are 9.2 ± 0.3 em! Hawaiian Islands. Place names for the islands and seamounts in the yr for the Hawaiian Chain and 7.2 ± 1.1 cm/yr for the Emperor Chain. A best fit through all the age data for both chains gives chain are shown in figure 1.1 (see also table 1.2) The Island of 8.6±0.2 em/yr. Alkalic rejuvenated-stage lava erupts on an Hawaii includes the active volcanoes of Mauna Loa, which erupted older shield during the formation of a new large shield volcano in 1984, and Kilauea, which erupted in 1986. Loihi Seamount, 190±30 km to the east. The duration of the quiescent period located about 30 km off the southeast coast of Hawaii, is also active preceding eruption of rejuvenated-stage lava decreases system and considered to be an embryonic Hawaiian volcano (Malahoff, atically from 2.5 m.y. on Niihau to <0.4 m.y. at Haleakala, reflecting an increase in the rate of volcanic propagation during chapter 6; Moore and others, 1979, 1982). Hualalai Volcano on the last few million years. Rejuvenated-stage lava is generated Hawaii and Haleakala Volcano on Maui have erupted in historical during the rapid change from subsidence to uplift as the vol times. Between Niihau and Kure Island only a few of the volcanoes canoes override a flexural arch created by loading the new rise above the sea as small volcanic islets and coral atolls. Beyond shield volcano on the ocean lithosphere. Kure the volcanoes are entirely submerged beneath the sea. Paleomagnetic data indicate that the Hawaiian hot spot has remained fixed during the last 40 m.y., but prior to that time the Approximately 3,450 km northwest of Kilauea, the Hawaiian hot spot was apparently located at a more northerly latitude. Chain bends sharply to the north and becomes the Emperor The most reliable data suggest about 70 of southward movement Seamounts, which continue northward another 2,300 km. of the hot spot between 65 and 40 Me. It is now clear that this remarkable feature was formed during The numerous hypotheses to explain the mechanism of the the past 70 m.y. or so as the Pacific lithospheric plate moved north hot spot fall into four types: propagating fracture hypotheses, and then west relative to a melting anomaly, called the Hawaiian hot thermal or chemical convection hypotheses, shear melting hypotheses, and heat injection hypotheses. A successful spot, located in the asthenosphere. According to this hot-spot hypothesis must explain the propagation of volcanism along the hypothesis, a trail of volcanoes was formed and left on the ocean 5
u.s. Geological Survey Professional Paper 1350
... w, , 8 VOLCANISM IN HAWAII
140· 160· 1BO· 120·
BERING SEA NORTH AMERICA
400
20'
EXPLANATION Age of oceanic crust (Mal
.0-40 .106-120
.40-73 0120-150
R73-106 .>150
FIGURE 1.2.-Magnetic anomaliesand structure of ocean floor crust in North Pacific modified from Hilde and others (1976} Hawaiian-Emperor Chain (black) crosscuts preexisting fracture zones and Mesozoic magnetic-anomaly sequence.
and small flows of lava richer in SiOz and FeO (these are the the bulk of the shield is built of tholeiitic basalt, but during declinin hawaiite and mugearite that characterize the alkalic postshield activity the magma compositions revert to alkalic basalt. The alkali stage). S. Powers (1920) noted that eruptive centers of nepheline preshield stage, like the alkalic postshield stage, produces only smai basalt on Kauai, Oahu, Molokai, and Maui were active long after volumes of lava, probably totaling less than a few percent of th the main volcano became quiet; he appears to have been the first to volcano. associate nepheline basalt with late-stage eruptions following an We have omitted the main caldera-collapse stage of Stearn erosional hiatus. (1966) from the eruption sequence because it can occur either durin: New insight into the preshield stage has come from recent the shield stage or near the beginning of the alkalic postshield stage studies of Loihi Seamount, a small submarine volcano located about The lava erupted may therefore be tholeiitic or alkalic basalt, or 0 30 km off the southeast coast of Hawaii. Its location, small size, both types. seismic activity, and fresh, glassy lava all indicate that Loihi is an active volcano and the youngest in the Hawaiian-Emperor Chain. GEOLOGY OF THE HAWAIIAN ISLANDS Some of the older lava samples recovered from Loihi Seamount are alkalic basalt and basanite, whereas the youngest lava samples Descriptions of volcanoes and their eruptions were made b: recovered are tholeiitic and transitional basalt. This observation led nearly all the earliest visitors to the Hawaiian Islands. Description Moore and others (1982) to conclude that Loihi Seamount, and of particular note are those of William Ellis (1823), George, Lon perhaps all Hawaiian volcanoes, initially erupt alkalic basalt. Later, Byron (1826), Joseph Goodrich (1826, 1834), and Titus COal I. THE HAWAIIAN·EMPEROR VOLCANIC CHAIN PART I 9
TABLE 1. I.-Hawaiian eruptive producb 100 HAWAIIAN RIDGE
Eruptive stage Rock types Eruption Volume rate (percent)
Rejuvenated -- alkalic basalt Very low basanite nephe 1ini t e ! nepheline melilitite 0 0 0 ~ 0 N 0 N, e ~ Postshield --- alkalic basalt Low ~ 0 transitional basalt ~ s ~ ankaramite ~ 0 hawaiite > 0 mugearIte . g ~ § -c benmoreite , ,, "~ trachyte I phone lite Shield ------tholeiitic basalt High 95-98 20 olivine tholeiitic basalt w picritic tholeiitic basalt o icelandite (rare) -c rhyodacite (rare) lalkalic basalt (1)
o 2000 4000 Preshield ---- basanite Low alkalic basalt DISTANCE FROM KILAUEA, IN KILOMETERS transitional basalt ltholeiitic basalt (7)
FIGURE 1.3.-Age of oceanic crust when overlying volcano formed, as a function lWright and Helz (chapter 23) suggest that the shield stage may of distance from Kilauea, for selected volcanoes in Hawaiian-Emperor Chain. include rare intercalated alkalic basalt and that the preshield stage includes tholeiitic basalt. We suspect that tholeiitic and alkalic Note offsets at fracture zones. Along Hawaiian Ridge both crust and volcanoes basalt occur intercalated during the transitions from preshield to increase in age 10 west so crustal age when volcanoes formed is roughly constant. shield stage and from shield stage to poatshield stage but that during On the other hand, Emperor Seamounts increase in age 10 north but crust the main shield stage only tholeiitic lava is erupted. decreases in age; thus age of crust when seamounts formed decreases from roughly 75 Ma at the bend to less than 40 Ma at Suiko Seamount.
milestone because it added detailed descriptions and chemical analyses of rocks from Hawaiian volcanoes other than Kilauea and Mauna Loa. (1840 and other letters until 1882). Many of their letters describing More detailed petrographic descriptions of lava from the the volcanoes were published in the American Journal of Science. islands were puhlished by S. Powers (1920). Soon afterward, Goodrich, in particular, provided detailed descriptions of the vol papers appeared by Washington (1923a, b, c) and Washington and canoes on the Island of Hawaii. None of the earliest descriptions Keyes (1926, 1928) with delailed accounls of the geology and however, included information about the mineralogy or petrology of petrology, new high-quality chemical analyses of lava from Hawaii the lava. and Maui, and a classification of Hawaiian volcanic rocks. Palmer The United States Exploring Expedition visited Hawaii in (1927, 1936) added geologic descriptions and petrography of lava 1840-41. The commander of the expedition published a narrative from Kaula and Lehua Islands, both of which are tuff cones of the (Wilkes, 1845) containing descriptions of caldera activity at Kilauea alkalic rejuvenated stage. Lehua Island is just one of several and new maps of both Kilauea and Mauna Loa calderas. James D. rejuvenated-stage vents associated with Niihau, whereas Kaula Dana, the geologist of the expedition, published a detailed report on Island sits atop a completely submerged shield. the geology of the areas visited by the expedition (Dana, 1849). These early, mainly descriptive and reconnaissance studies This report contains descriptions of lava flows including their were superseded by detailed mapping of the islands beginning in the mineralogy and flow morphology, in addition to numerous other 1930's. H.T Stearns and his coworkers, in a remarkable series of observations on the active and inactive volcanoes that make up the bulletins published by the Hawaii Division of Hydrography, pub islands. Later reports by Dutton (1884), J.D. Dana (1887, 1888, lished geologic maps and descriptions of Oahu (Stearns and 1889), Green (1887), and Brigham (1909) added details on Vaksvik, 1935; Stearns, 1939, I940h), Lanai and Kahoolawe eruptions and expanded the geologic observations to other islands. (Stearns. I940c), Maui (Stearns and Macdonald, 1942), Hawaii E.S. Dana (1877), Cross (1904), and Hitchcock (1911) (Stearns and Macdonald, 1946), Niihau (Stearns, 1947), and presented detailed petrographic descriptions of lava from the Molokai (Stearns and Macdonald, 1947). The bulletin on Keuai islands. Daly (1911) and Cross (1915) described the mineralogy by Macdonald and others (1960) completed the monumental map and petrology of Hawaiian lava flows at the time the Hawaiian ping job begun by Stearns; though Stearns did not coauthor the Volcano Ohservatory was established, and Jagger (1917) described report, he did much of the mapping and is an author of the map. activity in Halemaumau lava lake. The paper by Cross (1915) is a These maps and bulletins provide the geologic framework for all 10 VOLCANISM IN HAWAII
TABLE 1.2.-Ernptive stages represented on volcanoes of the Hawaiian-Emperor Chain (Volcano numbers from Bargar and Jackson (1974); numbers 0 and 65A added for consistency. Presence of slages: M, major unit; R, ran' or of small volume: X, present but c;lenl unkflown, A, known to be absent; -, unknown. (T), Iransitionallava probably erupted during late shield stage or caldera-collapse phase of that stage. For volcanoes from Kilauea through Nec::ker. data from detailed mapping and sampling; for remaining volcanoes, primarily from dredge and drill samples1
Eruptive Stages Volcano Preshield Shield postshield Rejuvenated Number Name (a1.kalie) (tholeiitic) (alkalic) (alkalic)
Hawaiian Islands
o Loihi ------ M M 1 Kilauea ------M A A 2 Mauna Loa ------ M A A 3 Mauna Kea ------ M M A 4 Hualalai ------M M A 5 Kohala ------M M A 6 East Maui ------ M M M 7 Kahoolawe ------ M R R 8 West Maui ------M R R 9 Lanai ------M A A 10 East Molokai ------ M M R 11 West Molokai ------M R A 12 Koolau ------M A M 13 Waianae ------ M M R 14 Kauai ------M R M 15 Niihau ------M R M 15A Kaula ------X X X
Northwestern Hawaiian Islands and Hawaiian Ridge
17 Nihoa ------ M 19 (Unnamed Seamount) X( T) 20 (Unnamed Seamount) -- X X 21 (Unnamed Seamount) -- X 23 Necker ------ M X X 26 La Perouse Pinnacles X 28 Brooks Bank ------ X( T) X 29 St. Rogatien Bank --- X 30 Gardner pinnacles --- X X 36 Laysan ------ X 37 Northampton Bank ---- X 39 pioneer Bank ------ X 50 Pearl and Hermes Reef X 51 Ladd Bank ------ X 52 Midway ------ M X 53 Nero Bank ------ X 57 (Unnamed Seamount) -- X 63 (Unnamed Seamount) --- x 65 Calahan ------X X 65A Abbott ------X( T)
Emperor Seamounts
67 Daikakuji ------ X 69 Yuryaku ------ X X 72 Kimmei ------ X 74 Koko (southern) ----- X M 76 Koko (northwest) ---- X 81 Ojin ------ X X 83 Jingu ------ X 86 Nintoku ------ X 90 Suiko (southern) ---- X 91 Suiko (central) ----- M X 108 Meiji ------M I. THE HAWAIIAN·EMPEROR VOLCANiC CHAIN PART I II subsequent studies of the islands and can also be used to put many of GEOLOGY OF THE HAWAIIAN RIDGE the earlier descriptions into a broader geological context. A number of derivative publications include summaries of the geology of the The Northwestern Hawaiian Islands were the focus of all islands by Stearns (1946, 1966), an overview of the petrography of geologic investigations along the Hawaiian Ridge west of Kauai lava from the islands by Macdonald (1949), and a summary of the until oceanographic techniques were applied to the area in the geology of the Hawaiian Islands by Macdonald and others (1983). 1950's. Geological descriptions of the leeward islands include those The brief geologic summaries in appendix 1. I have largely been of S. Powers (1920) for Nihoa and Necker Islands, and Wash extracted from the above publications. Additional unpublished ington and Keyes (1926) and Palmer (1927) for Nihoa, Necker, observations by ourselves are included for Hualalai, East and West Gardner Pinnacles, and French Frigates Shoal (LaPerouse Pinna Molokai, Kooleu. Kauai, and Niihau. cles). These reports cite earlier sketchy descriptions. Macdonald The maps of Stearns and coworkers separate rejuvenated-stage (1949) reexamined Palmer's samples and added more detailed lava from earlier lava, but do not subdivide shield and postshield petrography. The petrology of the basaltic basement of Midway lava on the basis of chemical composition. The eruptive stages that Atoll is described from two drill cores by Macdonald (1969) and are known to occur in each of the volcanoes of the Hawaiian Islands Dalrymple and others (1974, 1977), whereas the geology of the site are summarized in table 1.2. Evidence for the alkalic preshield stage is detailed by Ladd and others (1967, 1969), Paleomagnetic data exists only at Loihi Seamount. If this stage is present in all Hawaiian on flows and dikes from N ihoa and Necker Islands are given by volcanoes, it is completely buried by later, shield-stage tholeiitic Doell (1972), whereas similar data from the Midway drill core are lava. The tholeiitic shield stage is known to form the major portion of given by Gromme and Vine (1972). the subaerial and, we assume, the submarine part of each volcano. Marine geologic investigations of the Hawaiian Ridge began On the main islands, only Hualalai Volcano and Kaula Island do with Hamilton's pioneering work in 1957. Much subsequent work not have subaerial exposures of tholeiitic lava. Alkalic lava of the has focused on the structure of the oceanic crust in the vicinity of the alkalic postshield stage occurs relatively late in the eruptive sequence chain, but few cruises have actually been conducted that dealt mainly and has not yet developed on Loihi Seamount or Kilauea and with the geology of the Hawaiian Ridge. In the early 1970's, Mauna Loa Volcanoes. To the northwest of there it occurs on all Scripps Institution of Oceanography and the Hawaii Institute of volcanoes except Lanai and Koolau, although the volumes present Geophysics conducted cruises to the Hawaiian Ridge. Samples on Kauai, Niihau, Kahoolawe, and West Molokai are small. Some collected by these cruises are described in Clague (1974a, 1974h) volcanoes have predominantly mugearite, whereas others have pre and Garcia, Grooms, and Naughton (in press). Subsequent cruises dominantly hawaiite; these are called Kohala type and Haleakala to the area by the Hawaii Institute of Geophysics and the U.S. type, respectively, by Macdonald and Katsura (1962). Wright and Geological Survey are cited in appendix 1. 1. Clague (in press) propose two additional types: a Hualalai type Lava samples recovered from the Hawaiian Ridge and with a bimodal trachyte-alkalic basalt lava distribution and a Emperor Seamounts are more difficult to assign to volcanic stages Koolau type with little or no alkalic postshield lava present. because they are recovered by dredging and drilling or are collected Hawaiian volcanoes commonly have summit calderas and from small islets and the field relations are usually unknown or only elongate curved rift zones from which much of the lava issues. poorly known. Tahle l .2 summarizes the available data from the Summit calderas exist on Loihi Seamount (Malahoff, chapter 6; Hawaiian Ridge. Based on the sequence and volumes of lava in the Malahoff and others, 1982), Kilauea, and Mauna Loa. Each of Hawaiian Islands, we have assumed that tholeiitic basalt always these calderas is connected to two prominent rift zones. Not all represents the shield stage and that strongly alkalic, SiOz-poor lava Hawaiian volcanoes, however, had a summit caldera. West Molokai represents the alkalic rejuvenated stage. Differentiated alkalic lava Volcano, in particular, shows no evidence of ever having had a has been assigned to the alkalic postshield stage. Some alkalic basalt caldera. Flat-lying lava ponded inside a caldera is not exposed on occurrences could be assigned to either the alkalic postshield or Hualalai, Mauna Kea, Kohala, or Niihau, but former calderas are rejuvenated stages; they have been assigned on the basis of trace inferred at those volcanoes from geophysical data (see Macdonald element signatures and mineral chemistry using criteria outlined in a and others, 1983). later section of this paper. No lava samples have been assigned to the The formation and structure of the rift zones have been alkalic preshield stage because we assume that the small volumes of examined in an elegant paper by Fiske and Jackson (1972~ who such early lava have been buried by the later voluminous tholeiitic concluded that the orientation of the rift zones reflects local gravita lava of the shield stage. tional stresses within the volcanoes. Isolated shields such as Kauai The samples recovered by dredging are probably not represen and West Molokai had nearly symmetrical stress fields represented tative of the lava forming the bulk of the individual seamounts, but by generally radial dikes and thus have only poorly defined rift instead represent the youngest lava types erupted on the volcanoes. zones. The rift zones of these isolated volcanoes tend to align parallel This natural sampling bias should result in an overrepresentation of to the orientation of the chain, suggesting the influence of a more alkalic lava from both the postshield and rejuvenated stages. In regional stress field that also controls the orientation of the chain. In addition, selection of recovered samples for further study introduces contrast, the rift zones of the other volcanoes tend to be aligned another bias because the freshest samples are commonly alkalic lava, parallel to the flanks of the preexisting shields against which they particularly hawaiite, mugearite, and trachyte. With these biases in abut. mind, it is still possible to note general trends along the entire chain. 12 VOLCANISM IN HAWAII
Tholeiitic basalt and picritic tholeiitic basalt, similar to those of samples are alkalic basalt, hawaiite, mugearite, and trachyte similar the shield stage of subaerial Hawaiian volcanoes, have been to lava erupted in the Hawaiian Islands, but lava from Koko recovered from II seamounts, banks, and islands in the Hawaiian Seamount includes anorthoclase trachyte and phonolite that are Ridge west of Kauai and Niihau (table 1.2; appendix 1.1). The interpreted to have erupted during the alkalic postshield stage abundance of tholeiitic basalt from the Hawaiian Ridge implies that (Clague, 1974a). Lava of the rejuvenated alkalic stage has not been these volcanoes are genetically related to the Hawaiian Islands and identified from any of the Emperor Seamounts. that the general sequence of Hawaiian volcanism, in which tholeiitic basalt forms a major portion of each volcano, has occurred along the SUBSIDENCE OF THE VOLCANOES entire Hawaiian Chain.
Charles Darwin (1837, 1842) was the first to suggest that GEOLOGY OF THE EMPEROR SEAMOUNTS coral atolls might grow on subsiding platforms and that drowned Little was known of the geology of the Emperor Seamounts atolls and certain deeply submerged banks with level tops could be until quite recently. The chain was recognized as the continuation of explained by subsidence. Hess (1946) recognized that flat-topped the Hawaiian Ridge by Bezrukov and Udintsev (1955), but not submarine peaks, which he named guyots, were drowned islands. until 1968 were the first samples recovered from Suiko Seamount He thought that they were volcanic, bare of sediments and coral, (Ozima and others, 1970). These samples are dominantly, if not and had been planed off by erosion at sea level. He attributed their completely, ice-rafted detritus. Subsequent studies included a cruise depth to rising sea level caused by sediment deposition in the oceans. to the southern part of the chain by Scripps Institution of Menard and Dietz (1951) agreed with Hess that submergence was Oceanography in 1971 (ARIES Leg VII; Davies and others, primarily due to a rise in sea level, but they thought that local 1971, 1972), Deep Sea Drilling Project (DSDP) Site 192 on Meiji subsidence might also playa role. Hamilton (1956), in his classic Seamount (Creager and Scholl, 1973), DSDP Sites 308 and 309 study of the Mid-Pacific Mountains, which included a program of on Koko Seamount (Larson and others, 1975), a cruise by the dredging and coring, concluded that those (and other) guyots were Hawaii Institute of Geophysics (Dalrymple and Garcia, 1980), a formerly basaltic islands that had been wave and stream eroded and cruise by the U.S. Geological Survey in 1976 that surveyed the sites on which coral reefs subsequently grew. Their eventual sub for Leg 55 of DSDP (Dalrymple and others, 1980a), and Leg 55 mergence, he thought, was primarily caused by regional subsidence DSDP Sites 430, 431, 432, and 433 in the central part of the of the sea floor. It is now known that Darwin and Hamilton were chain (jackson and others, 1980). The Scripps Institution of basically correct about the steps leading to the formation of guyots, Oceanography cruise ARIES VII in 1971 and the Leg 55 DSDP and about the predominant role of subsidence in the process. cruise in 1977 were particularly successful, and most of our The Hawaiian-Emperor volcanic chain is an excellent example knowledge of the Emperor Seamounts is derived from these two of the gradual transformation of volcanic islands to guyots. From cruises. southeast to northwest there is a continuous progression from the The petrology of lava samples recovered by these two cruises is active volcanoes such as Mauna Loa and Kilauea through the described in Clague (1974a) and Kirkpatrick and others (1980), eroded remnants of Niihau, Nihoa, and Necker, through growing respectively. A detailed seismic interpretation of the carbonate caps atolls like French Frigates Shoal and Midway lslands, to deeply of many of the seamounts is given by Greene and others (1980), and submerged guyots like Ojin and Suiko. The progression can be overviews of the results of DSDP Leg 55 are given by Jackson and observed not only along the chain but within the stratigraphy of others (1980) and Clague (1981). individual seamounts. Drilling, dredging, and seismic observations Table 1.2 summarizes the available data on eruptive stages have shown conclusively that the atolls and guyots of the chain are represented by samples from the Emperor Seamounts, and details capped by carbonate deposits that overlie subaerial lava flows (see, are given in appendix 1.1 for individual volcanoes. We have for example, Ladd and others, 1967; Davies and others, 1971, assumed that tholeiitic basalt represents the shield stage and that 1972; Greene and others, 1980; Jackson and others, 1980). alkalic lava postdates the tholeiitic shield stage; only at Ojin and The subsidence of Hawaiian volcanoes with time results from Suiko Seamounts does drilling show that the alkalic lava overlies the thermal aging of the lithosphere and isostatic response to local tholeiitic flows. loading. The depth of the sea floor (and of volcanoes sitting upon it) Tholeiitic basalt and picritic tholeiitic basalt similar to those of increases away from spreading ridges because the lithosphere cools, the shield stage of subaerial Hawaiian volcanoes have been thickens, and subsides as it moves away from the source of heat recovered by drilling and dredging from six volcanic edifices in the beneath the ridge (Parsons and Sclater, 1977; Schroeder, 1984). Emperor Seamounts. The abundance of tholeiitic lava from the Detrick and Crough (1978) pointed out that the subsidence of many Emperor Seamounts is strong evidence that these volcanoes are islands and seamounts, including those along the Hawaiian genetically related to the Hawaiian Islands and Hawaiian Ridge. Emperor Chain, was far in excess of that which could be accounted Likewise, the general eruptive model for the Hawaiian Islands is for by this normal lithospheric aging or by lithospheric loading. apparently applicable to the Emperor Seamounts. They proposed that the lithosphere is thermally reset locally as it Alkalic postshield-stage lava has been recovered by dredging passes over a hot spot and that the excess subsidence is largely a and drilling from nine seamounts in the chain. In general these consequence of renewed lithospheric aging. I. THE HAWAIIAN-EMPEROR VOLCANIC CHAIN PART I 13
The Hawaiian-Emperor Chain rests on crust of Cretaceous GEOCHRONOLOGY AND PROPAGATION OF age (circa 120-80 Ma) for which the depth should be about VOLCANISM 5.5-5.9 km. The depth near Hawaii, however, is less than 4.5 km (fig. 1.4). The depth increases along the chain to about 5.3 km near EARLY WORK, LEGENDS AND DEGREE OF EROSION the Hawaiian-Emperor bend in a manner consistent with the thermal resetting hypothesis. Thus, the subsidence of Hawaiian volcanoes as According to Hawaiian legend, the goddess Pele first inhab they move away from the hot spot is in part a function of their ited Kauai, but then moved southeastward island by island to distance from the hot spot, that is, of the reset thermal age of the Kilauea Volcano, where she now resides (Bryan, 1915~ The lithosphere beneath the chain. The volcanoes are passively riding reasoning behind this legend is unknown, but it was probably based away from the Hawaiian hot spot on cooling and thickening in large part on the relative appearance of age of the various lithosphere that is subsiding at about 0.02 nun/yr. volcanoes. Many centuries after this legend originated, J.D. Dana Superimposed on the effect of crustal aging is subsidence (1849) rendered the first scientific opinion confirming the general age caused by the immense and rapid loading of the lithosphere by the progression implied by the legend. growing volcanoes (Moore, chapter 2). This effect is local, but Dana was not only the first geologist to conclude that the order while the volcano is active the rate of subsidence caused by loading of extinction of Hawaiian volcanoes was approximately from north may exceed that from lithospheric aging by more than two orders of west to southeast, he also recognized that the Hawaiian Chain magnitude. Moore (1970) found, from a study of tide-gage records included the islets, atolls, and banks that stretch for some distance to in the Hawaiian Islands and on the west coast of North America, the northwest of Kauai. Dana saw no reason to think that the that Hilo on the Island of Hawaii has been subsiding at an absolute volcanoes of the chain did not originate simultaneously: "No facts rate of 4.8 mm/yr since 1946. Recent data on drowned coral reefs can be pointed to, which render it even probable that Hawaii is of near Kealakekua Bay indicate an absolute subsidence rate for the more recent origin than Kenai" (Dana, 1849, p. 280} Their western side of Hawaii of 1.8 to 3 + mm/yr averaged over the past relative degree of erosion. however, provided ample evidence to 300,000 yr and also indicate that the rate may have accelerated indicate their order of extinction: "From Kauai to Mount Loa all during that time (Moore and Fornari, 1984). Moore's (1970) tide may thus have simultaneously commenced their ejections, and have gage data also show that absolute subsidence decreases systemati continued in operation during the same epoch till one after another cally away from the Island of Hawaii, with rates for Maui and Oahu became extinct. Now, the only burning summits out of the thirteen of 1.7 mm/yr and 0 mm/yr, respectively. Some of this decrease in which were once in action from Niihau to Hawaii, are those of Loa subsidence may be due to compensating uplift as the volcanoes are and Hualalai: we might say farther that these are all out of a number carried over the Hawaiian Arch, but an analysis of gravity data unknown, which stretched along for fifteen hundred miles, the length indicates that there is no appreciable viscous reaction to the sea of the whole range. This appears to be a correct view of the mount loads over time (Watts, 1978} Thus, it is probable that the Hawaiian Islands" (Dana, 1849, p. 280). Subsequent workers volcanoes are isostatically compensated within a few million years of agreed with Dana on the general order of extinction (for example, their birth, and that thermal aging of the lithosphere is the major Brigham, 1868; Dutton, 1884; Hillebrand, 1888; Hitchcock, cause of subsidence along the chain. 1911; Cross, 1915; Martin and Pierce, 1915; Wentworth, 1927; Hinds, 1931; Stearns, 1946), although the sequences they proposed invariably differed in detail (table 1.3) Of these various workers only Stearns (19461 who studied the Hawaiian Islands in more detail than any of his predecessors, had the sequence exactly correct as judged by present data. 4,----,--,--,------==--,------, The idea that the volcanoes of the Hawaiian Chain originated V> HAWAII MIDWAY I ••• , '"w simultaneously and only became extinct progressively seems to have tu ...... persisted until a few decades ago. Stearns (1946), for example, o mentions the lack of evidence to indicate when any of the Hawaiian "~ .. " 5 .... volcanoes began but shows all of the main shields except Hualalai ~ . and Kilauea erupting simultaneously at the end of the Pliocene I Ii: :....- 1- ••• (Stearns, 1946, p. 97, fig. 25). Two exceptions were Cross (1904) w ~iFZ- o - -MOFZ------__ and Wentworth (1927), who thought that the degree of erosion was 6L-_-l.______'__~______'__ _l__ _l__ _l__ __'__._J probably a function of when the volcanoes emerged above the sea as o 10 20 30 40 well as of the elapsed time since they ceased to erupt. Cross (1904, TIME SINCE REHEATING, IN MILLION YEARS p. 518) states: "It appears to me plausible to assume that the earliest FIGURE IA.-Minimum depth to sea-floor swell as a function of time since eruptions occurred at or near the western limit of this zone (the more reheating (or age of vokanoes along chain} Dashed line is predicted depth for than 1000 mile expanse of the island chain), and that in a general normal aging of lithosphere away from spreading ridge. Solid line is predicted depth for thermally reset lithosphere 45 km thick. MoFZ and MuFZ, Molokai way at least, the centers of activity have developed successively and Murray Fracture Zones, respectively. Modified from Detrick and Crough farther and farther to the east or southeast, until now the only active (1978) and Crough (1983). loci of eruption are those of Mauna Loa and Kilauea on the island of 14 VOLCANISM IN HAWAII
TABLE 1 3.-Earfy csnmcres of the order of extinction of the principal Hawaiian volcanoes [Criteria used are given beneath each source; volcanoes listed ill proposed order of extinction, oldest et tcp]
Dana ( 1849) Brigham (lsba) Dana (1888) Hillebrand (1888) Wentworth (1927) Hinds (1931) Stearns (1946 ) Erosion Erosion Erosion Floral divers ity Erosion Eros ion Erosion and stratigraphy
Kauai West Kauai, Kauai West Oahu, Kauai Koolau Waianae Kauai Waianae Niihau Waianae Molokai, East Oahu Kauai Koolau Waianae West Maui Waianae West MaUL Kcha l e , West Maui East Molokai Niihau Koolau Koolau East Kauai Kuhala Mauna K" West MaUL Kauai West Molokai Mauna K" West Molokai Koolau East Maui Mauna K" West Molokai East Molokai East Haui West Maui East Haui Hualalai Waianae East Molokai West Haui, Lanai Mauna Loa Kohala Mauna K" Mauna Loa, Kilauea East Maui Lanai Kahoolawe Koolau Hualalai Lanai West Maui, East Maui East Holokai Mauna Loa, Niihau, Kohala Kohala Mauna K" Kilauea West Holokai Kahoolawe Mauna K" Lanai, Kahoolawe Kahoolawe East Maui Hau l a l a i , Mauna East Maui Kohala Mauna K" Loa, Ki lauea Hualalai Hualalai, Mauna Hualalai Mauna Loa, Loa, Kilauea Mauna Loa, Ki Lauea Ki l a ue a
Hawaii. " He specifically noted the difference between his hypothesis have risen above the ocean long before, perhaps even in Mesozoic and that of Dana. time" (Hinds, 1931, p. 205), On the basis of geomorphic consid Estimates of the geologic ages of the Hawaiian volcanoes erations, Stearns (1946) thought that the volcanoes of the mam varied considerably among those early workers willing to hazard a Hawaiian Islands rose above sea level in the Tertiary. guess on the basis of the meager data then availahle. Dana (1849) thought it likely that the eruptions commenced as early as early Carboniferous or Silurian time; this estimate was based on the RADIOMETRIC AND FOSSIL AGES concept that the Earth had cooled from a molten globe producing fissuring and volcanism, the apparent lack of post-Silurian volcanism The first radiometric ages for Hawaiian volcanoes were deter in the interior of the North American continent, and the presump mined by McDougall (1963), who measured ages of 2.8 to 3.6 Ma tion that the oceans would cool after the continents. Cross (1904) for his Middle and Upper Waianae Series on Oahu (all K-Ar ages speculated that the western part of the leeward islands formed in the have been converted to the new constants; Steiger and Jaeger, 1977). early part of the Tertiary. Wentworth (1925, 1927) attempted to He also reported an age of 8.6 Ma for what he called the Mauna quantify erosion rates for several of the islands and estimated the Kuwale Trachyte of the Lower Waianae Series(?), an age that later extinction ages of some of the volcanoes as follows: proved to be incorrect, probably because of excess argon in the biotite analyzed (Funkhouser and others, 1968). In subsequent Lanai 0.15 Ma studies McDougall and Tarling (1963) and (primarily) McDougall Kohala 0.22 Ma (1964) reported K-Ar ages of lava from 7 of the principal Hawaiian Koolau 1.00 Ma volcanoes and concluded that the ages of the shield stages were Kauai 2.09 Ma approximately: On the basis of physiographic evidence, Wentworth doubted that Kauai 5.8-3.9 Ma any part of the Hawaiian group emerged above sea level before late Waianae 3.5-2.8 Ma Tertiary time. Hinds (1931), like Cross (1904), recognized that the Koolau 2.6-2.3 Ma atolls and banks of the leeward islands were the remnants of once West Molokai 1.8 Ma larger volcanoes: "The landscapes of the leeward group-the East Molokai 1.5-1.3 Ma volcanic stacks, the reef limestone and calcareous sand islands rising West Maui 1.3-1.15 Ma from submarine platforms, and submerged platforms from which no East Maui 0.8 Ma islands rise, represent the final stages in the destruction of a volcanic Hawaii (all 5 volcanoes) rhyolite Kilauea Volcano along the Hawaiian-Emperor trend. Because some (probably an erratic, see appendix 1.1) dredged from the northern of the volcanoes are unnamed and some seamounts and islands slope of Necker Island. consist of more than one major volcanic edifice, each dated volcanic In addition to the radiometric age data, there are paleontologic center is identified in the table with the number assigned to it by ages for several of the Hawaiian-Emperor volcanoes based on Bargar and Jackson (1974). The exceptions are Abboll Seamount, material recovered by dredging and drilling programs. In general, a small volcano between Cola han and Kammu Seamounts, and these ages postdate volcanic activity and are consistent with the Kaula Island, which were not previously numbered and to which we radiometric data. From southeast to northwest they include (I) an have assigned numbers 65A and 15A, respectively. age of 28-31 Ma for late Oligocene nannofossils in volcanogenic As can be seen from figure I. 5, the age data confirm the sediments at DSDP Site 311 on the archipelagic sediment apron of general age progression along the chain as first suggested by Dana an unnamed seamount (no. 58 of Bargar and Jackson, 1974) 240 (1849) and required by the hot-spot hypothesis of Wilsnn (1963a), km northwest of Midway (Hukry, 1975); (2) an age of 15-32 Ma and they show that the progression is continuous from Kilauea at (East Indies Tertiary stage Te) for larger foraminifers (Cole, 1969) least to Suiko Seamount, more than half way up the Emperor and smaller foraminifers (Todd and Low, 1970) in reef limestone Seamounts Chain and nearly 5,000 km from the active volcanoes above basalt in a drill hole al Midway Atoll; (3) an age of 39-41 of Mauna Loa and Kilauea. The data also substantiate the hy Ma for dredged late Eocene larger foraminifers from Kammu pothesis that the Emperor Seamounts are a continuation of the Seamount (Sachs, quoted in Clague and Jarrard, 1973); (4) an age Hawaiian Chain, as proposed by Christofferson (1968) and Mor of 50.5 ± 3. 5 Ma for early Eocene coccoliths in volcanogenic gan (1972a, b). sediments cored at DSDP Site 308 atop Koko Seamount (Bukry, 1975); (5) an age of 57-59 Ma for late Paleocene calcareous RATES OF VOLCANIC PROPAGATION nannofossils(Takayama, 1980) and pelagic foraminifers (Hagn and others, 1980) in sediments above basalt at DSDP Site 430 on Ojin In order to determine accurately the rate of volcanic propaga Seamount; (6) late Paleocene planktonic foraminifers and probable tion along the Hawaiian-Emperor Chain, we would like to know the early Eocene benthic foraminifers in sediments above basalt'at time that each tholeiitic shield volcano first erupted onto the sea floor, DSDP Site 432 on Ninloku Seamount (BUll, 1980); (7) an age of but such data clearly are not obtainable. What is available for the 59-61 Ma for middle Paleocene calcareous nannofossils in sedi dated volcanoes is one or more radiometric age on lava Rows erupted ments above basalt at DSDP Site 433 on Suiko Seamount (Tak during one or more stage of volcanic activity (see appendix 1.1). In ayama, 1980); and (8) an age of 70-73 Ma for lower order to calculate propagation rates, therefore, it is necessary to Maestrichtian nannofossils from sediments above basalt at DSDP adopt some consistent strategy for selecting the numerical age used to Site 192 on Meiji Seamount at the northern end of the Emperor represent the age of each dated volcano. Different authors have Seamounts (Worsley, 1973). None of these fossil ages is in conflict approached this problem in different ways. McDougall (1971) used with the radiometric data. the youngest age of tholeiitic basalt as representing the time of On the other hand, Menard and others (1962) describe cessation of volcanism for each dated volcano in the principal Miocene corals and pelagic foraminifers dredged from a submarine Hawaiian Islands. In contrast, Jackson and others (1972) and terrace 10 km southwest of Oahu. The authors note the difficulty in" Dalrymple and others (1980b, 1981) used the oldest age for assigning an age to these samples and state that the "planktonic tholeiitic volcanism as the best available approximation of the age of foraminifera Clobigcrinoidcs quadralobatcs [= C. trilobus auet.] the volcanoes. McDougall (1979) and McDougall and Duncan plexus suggest a lower limit of early Miocene. The upper age limit is (1980) adopted yet another approach and used the average age of less definitive" (Menard and others, 1962, p. 896). Present nomen tholeiitic shield volcanism. For table 1.4, we have chosen the oldest clature would identify these samples as Clobigcrinoides tnloba, which reliable ages for tholeiitic volcanism available, but the choice of ranges in age from early Miocene to Pleistocene (Kenneth and which ages to use is probably not critical when considering the data Srinivasan, 1983). Menard and others (1962) cite as additional for the chain as a whole. The reason is that the existing data on the evidence of the Miocene age of the sample the 60 percent of extinct rate of formation of Hawaiian volcanoes indicate that the tholeiitic coral species in the sample. We conclude that none of these criteria shields are probably built up from the sea floor in as little as unequivocally supports a Miocene age and no conflict exists between 0.5-1.5 m.y. (see summary in Jackson and others, 1972). This the ages of the reef and that of the underlying volcanic basement of amount of time is within the analytical uncertainty of the K-Ar ages 1.8-2.7 Ma. at about 20 Ma, or less than one-third of the way along the dated .....:.....:..;.:~,.
16 VOLCANISM IN HAWAII
TABLE 1.4.-Summary of K-Ar geochronology along the Hawaiian-Emperor volcanic chain
[Volcano number and distance [rom Bargar and Jackson (1974) and K, E. Bargar (written commun., 1978). 8 ...51 K-Ar age is oldest reliable age of tholeiitic basalt, where available: all data converted to new constants AE + x e ' = 0.581 X 10 - ID/ yr, A13 = 4.962 X 10- ID/ yr, 4UKJ K= 1.167X 10- 4 mol/mol]
Distance from Kilauea along Best Volcano trend of chain K-Ar age Data Num~ame (krn) (Ma) source Remarks
1 Ki l auea o 0-0.4 Historical tholeiitic eruptions 3 Mauna Kea 54 0.375*0.05 Samples from tholeiitic shield (Hamakua Volcanics) Koha La 100 0.43:1:0.02 Samples from tholeiitic shield (Pololu Basalt) Haleaka la 182 0.75*0.04 Samples from tholeiitic shield (Honomanu Bas a 1t) Kahoolawe 185 )1.03:1:0.18 Samples from alkalic postshield stage (upper part of Kanapou Volcanics) West MaUL 221 1.32:t0.04 4 Samples from tholeiitic shield (Wailuku Basalt) Lanai 226 1.28100.04 , Samples from tholeiitic shield (Lanai Basalt) 10 East Molokai 256 1.76±0.01 Samples from tholeiitic shield (lower member of East Ho Ic ka i Volcanics) II West Molokai 280 1.90:1:0.06 Samples from tholeiitic shield (lower part of West Molokai Volcanics) 12 Koolau 339 2.6:1:0.1 4,6 Ssmples from tholeiitic shield (Koolau Basalt) 13 Waianae 374 3.7:1:0.1 Samples from tholeiitic shield (lower member of Waianae Volcanics) 14 Kauai 5.1 :1:0.20 Sample from t ho l e i i t i c shield (Napali Member of Waimea Canyon Basalt) 15 Niihau 56' 4.89:1:0.11 Samples from tholeiitic shleld Lpan i au Basalt) 15A Kaula 600 4.0:1:0.2 21 Phonolite from p os r s h i el d stage (?) 17 Nihoa 780 7.2:1:0.3 9 Samples from tholeiitic shield 20 Unnamed 913 9.2:1:0.8 20 Dredged samples of alkalic basalt 23 Necker 1,058 10.3±0.4 9 Samples from tholeiitic shield 26 La Perouse Pinnacles 1,209 12.0±0.4 9 Samples from tholeiitic shield 27 Brooks Bank 1,256 13.0:1:0.6 20 Dredged samples of hawaiite and alkalic basalt 30 Gardner 1,435 12. 3±1 .0 20 Dredged samples of alkalic and pinnacles tholeiitic basalt 36 Laysan 1,818 19.9±0.3 10 Dredged sampl.es of hawaiite and mugearite 37 Northampton 1,841 26.6:1:.2.7 10 Dredged samples of tholeiitic Bank ba s a 1t 50 Pearl and 2,281 20.6:1:.0.5 II Dredged samples of phonolite, Hermes Reef hawaiite, and alkalic basalt Midway 2,432 21.7:1:0.6 12 Samples of mugeartte and hawaiite from conglomerate overlying tholeiitic basalt i n drill hole 57 Unnamed 2,600 28.0:1:.0.4 II Dredged samples of alkalic basalt 63 Unnamed 2,825 27.4:1:.0.5 II Dredged samples of alkalic basalt 65 Colahan 3,128 38.6:1:.0.3 13 Dredged samples of alkalic basalt 65A Abbott 3,280 38.7:1:0.9 13 Dredged samples of tholeiitic (?) basalt 67 Daikakuji 3,493 42.4:1:2.3 14 Dredged samples of alkalic basalt 69 Yuryaku 3,520 43.4:1:1.6 II Dredged samples of alkalic basalt 72 Kimmei 3,668 39.9:1:1.2 14 Dredged samples of alkalic basalt 14 Koko 3,758 48.1:1:0.8 14,15 Dredged samples of alkalic basalt, (southern) trachyte, ;;lnd phonolite 81 oj in 4,102 55.2:1:0.7 16 Samples of hawaiite and tholeiitic basalt from DSDP Site 430 83 Li ngu 4,175 55.4±0.9 17 Dredged samples of hawaiite and mugearite 86 Ni ntcku 4,452 56.2:1:0.6 16 Samples of alkalic basalt from DSDP Site 432. 90 Suiko 4,794 59.6olO.6 18,19 Single dredged sample of mugearite (southern) 91 Suiko 4,860 64.7oll.l 16 Samples of alkalic and tholeiitic (central) basalt from DSDP Site 433
Data sources: 1. Porter and others (1977) 12. Dalrymple and others (1977) 2. McDougall and Swanson (1972) 13 Duncan and Clague (l984) 3. Naughton and others (1980) 14. Dalrymple and Clague (1976) 4. McDougall (1964) 15. Clague and Dalrymple (l973) 5. Bonhomrnet and others (1977) 16. Dalrymple and others (l98oa) 6. Doell and Dalrymple (1973) 17. Dalrymple and Garcia (1980) J. McDougall (l979) 18. Saito and Ozima (1975) 8. G.B. Dalrymple (unpub. data, 1982) 19. Saito and Ozima (1977) 9 Dalrymple and others (1974) 20. Garc i e and others (1986b) 10. Dalrymple and others (l981) 21. Garcia and others (1986a) 11. Clague and others (1975) I. THE HAWAIIAN-EMPEROR VOLCANIC CHAIN PART I 17 80,-----,---,_----,---,,--_,-- ,.-__,-- ,.-__--, ,-__,--__-,
Meiji + / / Suiko 0 ,/ ,/ / 60 / Nintoku6/ "" Ojino6 ,/ / .. / =i / w Koko t::.. ./ o / -c / Z ~/ 0 Yurvaku o / c; 40 /+ t::. Kimmei
Laysan //'t::. 20 EXPLANATION o Tholeiitic lava /66,->...... 0 ...-6-: French Frigate Shoals 6 Alkalic lava Ale>/' o Rejuvenated lava Kauai 0::)"'" Nihoa + Paleontologic data / 2000 3000 4000 5000 6000 DISTANCE FROM KILAUEA, IN KILOMETERS
FIGURE 1.5.-Age of volcanoes in Hawaiian-Emperor Chain as a function of distance from Kilauea. Solid line is least-squares cubic fit (York 2) from table 1.5 and represents average rate of propagation of volcanism of 8.6 ± 0.2 era/yr. Dashed line is two-segment fit using data from Kilauea 10 Gardner and Laysan to Suiko (table 1.5). Radiometric data from table 1.4, paleontologic data discussed in text.
part of the chain. The question of which ages to use is in any case alkalic rejuvenated stage. In the principal Hawaiian Islands, lava moot for most of the volcanoes west of Kauai because so few suitable erupted during the rejuvenated stage may postdate the tholeiitic samples have been recovered that there is rarely a choice to make. shield and alkalic postshield stages by more than 4 m.y. A majority of the age data from islands and seamounts west of (McDougall, \964, G. B. Dalrymple, unpublished data, 1985). 50 French Frigates Shoal were obtained on alkalic rocks rather than on the main shield of volcano 63 may beseveral million years older than tholeiitic basalt. This is because the alkalic rocks, being younger indicated in table 1.4. than the tholeiitic basalt, are more likely to be recovered by dredging Previously, age-distance data along the Hawaiian-Emperor and drilling and are more resistant to submarine alteration than Chain have been regressed using a simple linear regression of age tholeiitic basalt. This bias toward ages of alkalic lava also probably (dependent variable) on distance (independent variable), either makes very little difference because the difference between the ages unconslrained (for example, McDougall; 1971, 1979, Jackson and of the postshield alkalic and youngest tholeiitic rocks is only a few others, 1972, McDougall and Duncan, 1980) or forced through the hundred thousand years in the Hawaiian Islands (McDougall, origin (for example, Dalrymple and others, 1980b, 198\). The 1964, 1969; Funkhouser and others, 1968, McDougall and Swan resulting volcanic propagation rates for the Hawaiian segment of the son, 1972; Doell and Dalrymple, 1973) and, presumably, in the chain have ranged from as little as 6 crn/yr (jackson and others, other volcanoes of the Hawaiian-Emperor Chain. For one unnamed 1975) 10 as much as IS cmlyr (McDougall, 1971, Jackson and volcano on the western Hawaiian Ridge (63 in appendix 1.1 and others, 1972), although most recent estimates have been between 8 table 1.4) the only data available are from lava erupted during the and 10 cmlyr (McDougall, 1979; McDougall and Duncan, 1980, 18 VOLCANISM IN HAWAII
Dalrymple and others. 1981 ~ Simple linear regression models have regressions and the two simpler regression models for v the disadvantages that they presume no error in distance and they do segments of the Hawaiian-Emperor Chain are given in tabk not take into account the experimental errors of individual deter For the entire chain, the average rate of volcanic propagal minations. 8.6±O.2 crn/yr with an intersection (that is, theoretical zero We have treated the data in table 1.4 using a two-error cubic fit 89 km northwest of Kilauea using the York 2 regression. The: (York 2), which allows for errors in both age and distance and regression models yield similar, though slightly lower, vah weights the data accordingly (York, 1969). Errors for the age propagation rate. determinations are straightforward and are either provided in the Rates of propagation for the Hawaiian segment of the original references or have been estimated by us from the array of that is, Kilauea through Abbott, have been calculated using be data available on an individual volcano. Jackson and others (1975) maximum and minimum ages of tholeiitic volcanism. The rest estimated the cumulative errors in distance to be about 1.5 km at not vary with model and range from 8.6 to 9.2 cm/yr Kilauea to as much as 20 ken near the western end of the Hawaiian comparison. we have included comparable calculations usir Chain. We have interpolated and extrapolated these values to find average ages of McDougall (1979~ The resulting rates are errors for the distances in table 1.4. The results of both the York 2 what higher than the rates calculated from either the maximt
TABLE 1.5.-Rates of proP Data Simple regression York 2 Chain segment source Forced through fit Unc o n s t r uc t e d origin Hawaiian-Emperor --- tab l e 1.4 7.8±0.2 8.2±0.1 8.6±0.2 ( 175, 0.992) ( 89) Hawaiian ------tab l e 1.4 8.6±0.3 9.1±0.2 9.2±0.3 (maximum ages) 002, 0.985) (80) McDougall, 1979 9.4±O.3 9.9±O.2 1l.3±O.1 ( average ages) ( 91 , 0.994) (3) appendix 1.1 8.6±O.3 9.1±0.2 9.I±O.3 (minimum ages) 019, 0.986) ( 9)) Emperor ------table 1.4 6.5±O.8 7.9±O.2 7.2±1.1 Kilauea to Gardner - tab l e 1.4 9.9.0.3 10.6.0.3 9.6±O.4 (57, 0.992) (3) Laysan to Suiko ---- tab Ie 1.4 6.9±O.4 8.I±O.2 6.8±O.3 (0.971 ) Gardner to Waianae - table 1.4 9.5±O.4 IO.I±O.2 IO.HO.8 (54, 0,993) (9 ) I. THE HAWAIIAN·EMPEROR VOLCANIC CHAIN PART I 19 minimum data, but the difference is largely a consequence of the case; the volcanoes are irregularly spaced within a band some differences in the data sets, the ones in table 1.4 and appendix 1. I 200-300 km wide, indicating clearly that volcanic propagation is being more current. irregular. Rates calculated for the Emperor Chain, that is, Daikakuji Although some of the irregularities in the age-distance data no through Suiko, are markedly lower than for the Hawaiian Chain, doubt reflect dating errors and differences in the stage of volcanism ranging from 6.5 to 7.2 cm/yr when not forced through the origin. sampled, some of the deviations appear to be larger than can Separate rates for these two major segments of the chain are only reasonably be attributed to these causes. For example, the ages of meaningful. however, if there was a rate change at the time of Laysan and Northampton Bank should differ by only about 0.3 formation of the bend. This hypothesis can be tested by using the m.y, rather than the 6.7 m.y. indicated by their measured ages. A linear equations found from the York 2 regressions to predict the age similar discrepancy occurs in the ages of volcanoes near the bend of the bend, which we estimate to be 3,451 km from Kilauea at the (table 1.4; fig. 1.5). There are also volcanoes in the chain that position of volcano 68. The predicted ages for the bend are 36.7 appear to have been active simultaneously even though they were Ma and and 43.0 Ma for the Hawaiian and Emperor segments, separated by distances of hundreds of kilometers. Examples include respectively. The Hawaiian prediction, which is similar to the value Laysan, and Pearl and Hermes, as well as Midway and North of 37.8 Ma found by McDougall (1979\ differs significantly from ampton. Indeed, Mauna Loa, Kilauea, and Loihi are currently the measured bend age of 43.1 ± 1.4 Ma as determined from the active, erupting tholeiitic basalt, and are separated by more than 80 ages of Daikakuji and Y uryaku Seamounts. This suggests that if km. there was a significant change in volcanic propagation rate it did not The primary reason tbat Jackson and others (1972) suggested occur at bend time, but some time after, a conclusion also reached by short-term nonlinearities in propagation rates was the pronounced Epp (1978\ curvature in the age-distance data from the volcanoes of the principal For some time, it has been apparent to us that a change in rate Hawaiian Islands. When plotted as a function of distance from near or before the time of formation of Midway is consistent with the Kilauea, the ages for these volcanoes clearly indicate an acceleration available data (Dalrymple and others, I980b). For example, the fits of volcanic propagation over the past 5 m.y. {Jackson and others, of the data for the chain segments Kilauea-Gardner and Leysan 1972~ This curvature is also one reason that virtually all regressions Suiko are slightly better than the fits for the Hawaiian and Emperor intersect the distance axis northwest of Kilauea (table 1.5) and segments (table 1.5; fig. 1.5). The two former lines intersect near predict a negative age for that volcano. McDougall (1979) has Gardner Pinnacles at an age of about 18 Ma. Epp (1978) argued that the curvature is caused by a bias toward young ages for concluded that a rate change occurred around 20-2S Ma. We have the less eroded volcanoes, but this cannot be so. Even though tried various ways to determine the most likely time for a change in Kohala Mountain is relatively uneroded, it is deeply incised on the the rate of volcanic propagation, including correlation with eruption windward side by several canyons whose floors are near sea level, volumes along the chain (see section below on eruption rates) and and it is unlikely that further erosion will expose lava significantly age-predictive models for the central parts of the chain, but we are older than is now exposed. In addition, the rapid subsidence of not convinced that the results are meaningful. We can only conclude Hawaii (Moore, 1970) may carry tbe oldest subaerial lava flows that the data imply, but do not require, a change of rate sometime below sea level before they can be exposed by erosion. Similar after the formation of the Hawaiian-Emperor bend and before or arguments can be made for West Maui, Lanai, Kahoolawe, East near the time of formation of Laysan Volcano. Molokai, and Koolau Volcanoes, where lava deep within the In addition to the possibility of a major change in the volcanic subaerial part of the tholeiitic shield has been exposed by marine or propagation rate, as discussed above, there are also indications of stream erosion or by faulting. short-term departures from linearity. Short-term changes in the We have plotted the known age range for tholeiitic shield, volcanic propagation rate were first proposed by Jackson and others alkalic postshield, and alkalic rejuvenated-stage volcanism for the (1972) to explain the apparent acceleration of propagation during principal Hawaiian volcanoes in figure 1.6, from which the accelera the past 5 m.y. or so. They did not suggest that short-term variations tion of volcanic propagation over the past 3-5 m.y. is evident. It is in propagation rate reflected variations in relative motion of hot spot also clear from this figure that the curvature in the age-distance data and plate. Shaw (1973) and Walcott (1976) proposed thermal is not a function of which eruption stage, tholeiitic shield or alkalic feedback mechanisms to account for such variations without varying postshield, is chosen to represent the age of the volcanoes. Further the relative rate of motion between the hot spot and the Pacific plate more, a bias toward younger ages for the less eroded volcanoes, (see section below on models). Nonlinear models have been disputed taken to include Kilauea through Haleakala, cannot produce the by McDougall (1979) and McDougall and Duncan (1980), who curvature because older ages for these volcanoes would exaggerate, argue that linear regressions fit the Hawaiian data so well that no not lessen, the apparent acceleration. Thus, the acceleration of other model needs to be considered. volcanic propagation in the principal islands, as proposed by It seems obvious to us from the geometry alone, however, that Jackson and others (1972), appears to us to be real. the volcanic propagation rates must be nonlinear in detail. If this While the overall rate of propagation of volcanism along the were not so, then either the volcanism would have formed a ridge chain (or at least major segments of it) may be linear and reflect the rather than individual volcanoes, or the volcanoes in the chain would relative motion between the Pacific plate and the Hawaiian hot spot, be spaced in proportion to their ages along a single line. Neither is there also appears to be ample justification for retaining nonlinear 20 VOLCANISM IN HAWAII 6,-r------,------,-----,------.-----~----~ EXPLANATION ~ Alkalic rejuvenated-stage volcanism ill Alkalic postshield-stage volcanism 5 W Tholeiitic shield-stage volcanism 4 "~ ur to m ~ m ~ "• m ":I: m • m ~ a ~ ""m s: m c c 0 "0 0 m m m :1 "" ~ •0 :1 ~ ~" "" ~ ~ ~ ~ ~ a 0 0 ~ 0 100 200 300 400 500 60 DISTANCE FROM KILAUEA, IN KILOMETERS FIGURE 1.6.-Known durations of tholeiitic shield. alkalic posishield, and alkalic rejuvenated-stage volcanism for dated volcanoes of principal Hawaiian Islands. Anj lines indicate overlapping or uncertain ages or overlapping volcanism. Data from sources discussed inappendix 1.1. Data for Niihau and for Kauai (Koloa Volcanics) from G.B. Dalrymple (unpublished data, 1985~ propagation on a small scale as a working hypothesis. It is unlikely for the North Pacific (Chase and others, 1970) and their 19 that the cause of this nonlinear propagation, if real, will be known derivative (Chase and others, 1973) are probably still tbe b until more is learned about the hot-spot mechanism. published sources available. An updated bathymetric chart for Emperor Seamounts (Clague and others, 1980) was based on data used by Cbase and others (1970) and additional geophysi ERUPTION RATES ALONG THE CHAIN profiles collected between 1970 and 1979; recently publisl The bathymetry of the chain as a whole is not well known, bathymetry for much of the central part of the Emperor Seamou particularly for the western Hawaiian Ridge, and the 1970 charts (Smoot, 1982) is based on previously classified Navy multibe I. THE HAWAIIAN·EMPEROR VOLCANICCHAIN PART I 21 data. The gross structure of the Emperor Seamounts is little extreme products of Hawaiian volcanism, nepheline basalt and changed in the later charts, but the shapes and locations of some trachyte, may appear either at the close of the main volcanism or in a individual volcanoes changed dramatically (fig. 1.7). later phase after extensive erosion." Bargar and Jackson (1974) compiled volume data along the This viewpoint, that there was a single primary Hawaiian chain and identified individual volcanic centers and their rift systems magma from which the varieties of lava evolved by means of using the bathymetry of Chase and others (1970). From the more differentiation, was popular well into the 1960's. H. Powers (1935) accurate muhibeam data it is dear that many of the volcanic centers expressed a similar view, although he showed that fractional crys and rift zones identified by Bargar and Jackson are incorrect in tallization alone could not explain the differentiation of Hawaiian detail. Because the number and general sizes of the volcanoes change basalt. Macdonald (1949) proposed that the sole primary little on the later charts, we have used Bargar and Jackson's volume Hawaiian lava was olivine basalt, although his calculated average estimates rather than engage in the laborious process of calculating included both alkalic and tholeiitic olivine basalt analyses (which he new ones from the newer data. We suspect that the volumes based on did not distinguish at that time). He also proposed that andesine multibeam data would vary relatively little from those of Bargar and andesite (hawaiite), oligoclase andesite (mugearite), and trachyte Jackson. were successive differentiates from an olivine basalt parental lava. The cumulative volume of the volcanoes is plotted in figure 1.8 This view is now known to be incorrect because Macdonald's against distance from Kilauea beginning at Tenchi Seamount, 500 calculated olivine basalt was basically a tholeiitic basalt in composi km north of Suiko. It is clear that the volume of eruptive products tion. He further inferred that picritic basalt of the oceanite type per unit distance along the chain has not been constant over the past (here termed picritic tholeiitic basalt) formed by the accumulation of 70 million years. olivine and that ankaramite was not an oceanite that simply accumu We have calculated dVldx, where V is volume and x is lated clinopyroxene. This last idea is correct, ankaramite being distance, for segments of the chain. which are summarized in table alkalic in composition whereas picritic basalt of the oceanite type is 1.6. Also listed are dxldt. where t is time. calculated from the age tholeiitic. In order to differentiate ankaramite and nepheline basalt relations along the chain, and the derived quantity dVldt for from the parental nlivine basalt. Macdonald (1949) proposed that segments along the chain. These calculations clearly show that the limestone assimilation and selective remelting (wall-rock assimilation) volumes erupted per unit distance along the chain and per unit time were important processes. He correctly inferred that the dunite increase from the Emperor Seamounts to the Hawaiian Ridge and xenoliths so common in alkalic lava from the postshield and rejuve to the Hawaiian Islands. The present-day eruption rate for Kilauea nated stages formed by accumulation of olivine followed by alone, when compared to eruption rates along the Hawaiian Ridge recrystallization. and Emperor Seamounts, demonstrates that the Hawaiian hot spot Tilley (1950) recognized thai the bulk of the primitive shields is presently producing large volumes of lava at the greatest eruption was made of tholeiitic basalt and that alkalic rocks erupted only rates in its known history. The average eruption rate from Hualalai during the declining stages of activity. He proposed that alkalic to Kilauea is 5 times that for the islands as a whole and nearly 22 olivine basalt was derived from tholeiitic basalt by crystal fractiona times the rate for the entire chain. The only section of the chain tion. H. Powers (1935) had, however, earlier noted that primitive where volumes do not increase toward the present is the westernmost lava was silica saturated, whereas the late differentiated lava was section of the Hawaiian Ridge, which formed immediately following silica undersaturated; he argued that these lavas could therefore not the change in plate motion recorded as the Hawaiian-Emperor be simply related to one another by crystal fractionation. bend. This change in plate motion was followed by a virtual New concepts important to understanding the origin of cessation of volcanic activity that lasted for nearly 10 m.y. Hawaiian lava were introduced by H. Powers (1955). He clearly established that the abundant rocks termed olivine basalt in the PETROLOGY OF THE HAWAIIAN·EMPEROR shields are silica saturated and noted that they are compositionally VOLCANIC CHAIN distinct for individual volcanoes. He proposed the concept of magma batches to account for the subtle differences between the lava EARLY WORK, LAVA SERIES AND DIFFERENTIATES of different shields. He also reiterated that olivine basalt erupted Early observers of Hawaiian eruptions rather uniformly agreed during the declining stages of activity is silica undersaturated. His that the lava originated "in the bowels of the earth." As time discussion of fractionation trends for tholeiitic and alkalic basalt is progressed this view was expanded upon, but it was not until the nearly identical to present-day views. He further recognized that 1950's and 1960's that the lava source and the processes generating earthquakes associated with volcanic activity gave a minimum depth the various lava types were discussed in detail. S. Powers (1920) of magma generation which he took to be 48-56 km (30-35 miles), proposed that nepheline basalt and trachyte were formed by dif His estimates of the source rocks that could be melted to produce ferentiation of basaltic magma because of their occurrence late in the basalt and of the causes of melting provided a framework for eruptive sequence. He wrote (5. Powers, 1920, p. 280): "Each experimental research for many years. In particular, he noted that volcanohas arisen at an intersection in a fracture system in the earth's basalt could be generated at depth by wholesale melting of rocks of crust, has been fed from the same primal source, and has finally lost basaltic composition or by partial melting of peridotite. The models connection with that source. When this takes place differentiation of melting he considered all assumed that it was caused by an may proceed in the magma chambers of large volcanoes and the increase in temperature. He dismissed exothermic nuclear processes 22 VOLCANISM IN HAWAII Chase and others (1973) Clague and Smoot others (1980) 11982) 45· 40" 40· 40· Ojin 170· 170" 170" CONTOUR CONTOUR CONTOUR INTERVAL INTERVAL INTERVAL 500 FATHOMS 500 METERS 500 FATHOMS o 100 200 KILOMETERS I I FIGURE 1.7.-Comparison of bathymetry of central Emperor Seamounts from Chase and others (1973; left), Clague and others (1980bj center) and Smoot (1982; right} General size and shape of seamounts were fairly well mapped by bathymetric sounding (left and center), but multibeam bathymetry (right) adds wealth of detail. Contour intervals are 500 fathoms for left and right figures and 500 m for center figure. I. THE HAWAIIAN·EMPEROR VOLCANIC CHAIN PART I 23 Kuno and others (1957) clearly demonstrated that closed TABLE 1.6.-Eroptive rales along the Hawaiian-Emperor Chain [Volume/distancedala from figure 1.8; propagation rate data from table 1.5. except for Kilauea to Hualalai; recent data for Kilauea from Dzurisin and others (1984 ~ based on combined eruption-intrusion rate] g eguent Volume/distance, Propagation rate, Eruption rate dV/dz (10) km3/km) dx/dt: (km/m,y,) dV/dt (103 km)/m,y,) Kilauea (1956-1983) 85 Kilauea to Hualalai 1,500 250 290 Hualalai to Waianae 400 101 40 Hawaiian Islands (0-5.5 Ma) 56 Waianae to Gardner Pinnacles 190 101 19 Gardner Pinnacles to volcano 57 200 68 14 Volcano 57 to Hawaiian-Emperor bend 20 68 1 Emperor Seamounts 160 J2 t2 Average for entire chain 13 24 VOLCANISM IN HAWAII type volcanoes between the tholeiitic shield lava and the later alkalic Macdonald (1968) also calculated average compositions of postshield-stage lava and proposed that volatile transfer might be an Hawaiian lava from the different eruptive stages. His average important differentiation process. They discussed thoroughly the compositions, recalculated on a dry-reduced normalized basis, are fractionation sequences of bothalkalic and tholeiitic lava and related presented in table 1.7. These averages clearly show that lava of the the Mauna Kuwale rhyodacite to tholeiitic lava of the Waianae tholeiitic shield stage is silica saturated and that of alkalic postshield Range. and rejuvenated stages is silica undersaturated. The presence of The years 1964-68 produced new insights from a variety of normative hypersthene in the mugearite, benmoreite, and trachyte, studies. The first isotopic data from Hawaiian lava (Lessing and which are derived from undersaturated alkalic basalt, reflects frac Catanzaro, 1964; Hamilton, 1965; Powell and DeLong, 1966; tionation of Fe-Ti oxides, which enriches the residual melt in silica. "Iatsumoto. 1966) clearly demonstrated that the source rocks for Rejuvenated-stage alkalic basalt contains greater than 5 percent Hawaiian lava were heterogeneous. Experimental studies at high normative nepheline, and average nephehnite and nepheline melilitite pressure and temperature (for example, O'Hara, 1965; Green and contain normative leucite. Alkalic basalt of the preshield and Ringwood, 1967) added new data bearing on the mineralogy of rejuvenated stages are similar in composition. The preshield Loihi potential source rocks and the physical conditions of melting. At the Seamount averages are calculated from Moore and others (1982), same time, trace-element data began to be used to evaluate Frey and Clague (1983) and D.A. Clague (unpub. data, 1985). Hawaiian petrogenetic processes (Schilling and Winchester, 1966; Gast, 1968). Studies of Hawaiian xenoliths (White, 1966) added XENOLITH DISTRIBUTIONS to the abundant new data being used to evaluate the petrogenesis of Hawaiian lava and the nature of the source rocks. This period marks In a detailed analysis of the xenolith populations in Hawaiian a transition from relatively qualitative models of petrogenesis to lava, Jackson (1968) subdivided the xenoliths into dikes and sills, modern quantitive modeling and testing of basalt petrogenesis. To a cumulates, and metamorphic rocks. His breakdown of the relative great degree present day petrogenic models are based on these same abundances and types of xenoliths is given in table 1.8, modified to types of data and similar quantitative modeling techniques. include xenoliths found in Loihi Seamount alkalic preshield lava. However, because modern isotopic and trace-element data are more Jackson noted that only those xenoliths with metamorphic textures accurate and precise, the models proposed are more refined and could represent either mantle source rocks or mantle residua left after complex. partial melting. The dikes, sills, and some, but not all, of the Macdonald (1968) followed Green and Ringwood (1967) cumulate rocks are cognate or from shallow depths. The cumulate and proposed that the tholeiitic, alkalic, and nephelinitic lava types xenoliths from Hualalai Volcano appear to come from a variety of were derived from a single parent magma of olivine tholeiitic basalt sources, including cumulates formed as part of oceanic crustal layer composition. He proposed that the compositional variations reflect 3, cumulates of tholeiitic Hawaiian shield lava, and cumulates of lava the depth at which fractional crystallization occurred with tholeiitic from the alkalic postshield stage (D.A. Clague, unpub. data, basalt fractionated at shallow depths, alkalic basalt at moderate 1985). The single cumulate xenolith from Loihi Seamount presum depths, and nephelinitic lava at depths of several tens of kilometers. ably represents a cumulate of ocean crustal layer 3. He further argued that the primary magma is olivine tholeiitic basalt Jackson and Wright (1971) proposed that the abundant dunite rather than tholeiitic basalt because most lava has lost olivine, which xenoliths in the Honolulu Volcanics represent residue left after accumulated within the magma chambers to form the high-density melting the mantle to form Koolau shield tholeiite, an interpretation masses discovered by gravity surveys (summary and references in with which we disagree. Jackson and Wright (1971) inferred that the Jackson and others, 1972) Macdonald (1968) noted that the garnet lherzolite and lherzolite found only in alkalic lava from the highest temperature lava from the Kilauea Iki eruption contained rejuvenated stage were potential mantle source rocks. The difference 27 -30 percent olivine and proposed that this closely approximated in xenolith populations for the three alkalic eruptive stages is striking primary magma. Wright (1973) calculated the bulk composition of since only the lava from the preshield stage and rejuvenated stage the same eruption and proposed it as a representative parental (but contain xenoliths that formed at depths greater than about 20 km. not necessarily primary) composition for Kilauea tholeiitic basalt. Although it would be useful if these xenolith populations reflected the Macdonald (1968) presented quantitative models showing that mantle through which the lava ascends, it seems more likely that they ankaramite is alkalic basalt plus olivine and clinopyroxene and that reflect the development of shallow magma storage reservoirs, which hawaiite is alkalic basalt minus olivine, clinopyroxene, plagioclase, act as hydraulic filters and remove xenoliths carried up from greater and magnetite. This type of mass-balance approach was later depths in much the same way as lakes remove sediment from rivers. refined by Wright (1971) and Wright and Fiske (1971) to demon Lava stored in a shallow magma reservoir, either within a feVl strate the roles of fractionation and hybridization in generating basalt kilometers of the surface or at the base of the oceanic crust, lose an~ at Kilauea and Mauna Loa. The debate about whether primary xenoliths they may have acquired during ascent and from this poin tholeiitic magma is olivine rich or olivine poor continues today (see can only entrain xenoliths that occur at shallower levels in th. Wright and Helz, chapter 23; Wright, 1984; Budahn and Schmitt, volcanic system. However, lava of the preshield and rejuvenater 1984). Extreme compositions are liquids with 20 percent MgO stages erupts in small volumes at infrequent intervals and probabf (Wright, 1984) and average tholeiitic basalt with 9 percent MgO no shallow magma storage reservoirs exist. During the shield stage (Powers, 1955). tholeiitic lava erupts in large volumes at frequent intervals from ' I. THE HAWAIIAN-EMPEROR VOLCANIC CHAIN PART I 25 TABLE 1.7. -Average compo~itions and norms of major Hawaiian lava types [All ~gures in weight percent; __ nol present. Normative components calculated with original FeO/FczOl ratios. See Macdonald (1968) for remainder ofnorms for all bUIthe alkalic preshield stage. Data for alkalic preshield stage from Frey and Clague (1983) and D.A. Clague (unpub. data, 1985)] Tholeiitic Stage Alkalic preshield shield Alkalic postshield Alkalic r e i uvena ted e " " ~ ~ .. ~ u "> .•>~ ~ ~ Lava type .. ~ .. ~ .. ~ • • .. 0 • 0 " " ~•" ~• ~ .. ~~• ~ ~ -e ~ ~ ~ ~ .~ ~ 0 " o • -" ~ • .. • • "• ~ • ~ ~ u ~ " ~ 0 ~•" ...... ~ ~• ~ •" " ~ ~ " -" .. " ~ .• ~ .. " o • .. .. " " ~ ~ ~ ..~ ..~ ~ " .. u " e u o .s ~" " .. ~ " .. .. ~ ~~• .. " e-, " ~ ...... ~ . " .. ~ .. .• " ~ .. 0 c .. 0 • .• " "0 -" ~-" " ~-" " • u -" .. "o ~ • • "0 ~ • • •) ~ • •" "0. ~ .~ ~ " ;'j •" " " , u • " U H ;;;'" • 0. '" '" • "" H • 05 " '" 05 "" " '" " '" " " '" z" " Chemical composition Si02 ------48.4 48.3 45.6 43.5 46.7 50.0 44.6 45.9 48.6 52.1 58.3 62.8 45.2 44.6 40.6 37.8 AI 13.6 11.6 14.1 16.1 17 .1 12.8 12.8 Z0 3 ----- 12.2 11.1 8.5 12.2 14.9 18.0 18.3 11.6 11.2 reO' ------12.0 12.3 12.4 13.6 12.1 11.3 12.6 13 .0 12.2 10.0 7.5 4.5 12.4 12.5 13 .3 14.6 MgO ------11.2 7.5 13.5 12.2 20.9 8.5 13.1 7.9 4.9 3.3 1.6 .4 11.5 11 .3 12.4 13 .0 CaD ------11.0 11.4 10.4 11.4 7.4 10.4 11.6 10 .6 8.1 6.2 3.6 1.2 11.5 10.7 13.1 14.1 NaZO ------2.1 2.7 2.5 3.2 1.6 2.2 1.9 3.0 4.3 5.5 6.0 7.5 2.7 3.6 3.9 4.2 K~O ------.4 .7 .8 1.3 .3 .4 .7 1.0 1.5 2.1 2.9 4.3 .9 1.0 1.2 1.0 T102 ------2.3 3.1 2.7 3.1 2.0 2.5 2.7 3.0 3.4 2.4 1.2 .5 2.3 2.6 2.9 2.9 P205 ------.2 .3 .3 .5 .2 .3 .3 .4 .7 1.1 .7 .2 .5 .5 .9 1.1 MnO ------.2 .2 .2 .2 .2 .2 .2 .2 .2 0.2 .2 .2 .2 .2 .2 .1 Normative composition Q ------2.2 N' ------2.7 11.8 2.6 2.6 0.3 6.0 10.5 17.3 18.7 Lc ------5.7 4.8 Ny ------14.3 6.3 15.9 21.5 2.7 4.0 .4 01 ------10.5 5.9 23.1 17.7 29.5 22.2 13.2 6.7 2.1 19.3 17.9 14.9 20.2 shallow magma storage reservoir and perhaps a deeper staging zone an intermediate staging area at 20-30 km, similar to that beneath (see review by Decker, chapter 42). During the alkalic postshield Kilauea, acts as an effective filter that removes any lherzolite or stage, lava erupts in small volumes at infrequent intervals, though in garnet peridotite xenoliths. Lava may fractionate in this zone and, larger volumes and at more frequent intervals than during the alkalic upon movement to the surface, entrain xenoliths of ocean crust rocks preshield or rejuvenated stages. During this stage, lava apparently and cumulates formed in earlier volcanic stages at shallow depth. resides in reservoirs below the base of the oceanic crust (Clague and The presence of xenoliths that originate at great depth in alkalic lava others, 1981) for time periods sufficient for the dense peridotite of both the preshield and rejuvenated stages implies that neither xenoliths to settle out. Tholeiitic lava at Kilauea passes through two shallow nor intermediate staging area ads as an effective filter in suchfilters. one an intermediate-depth (20-30 km) staging area, the these stages. The near-primary character of the host lava also second a well-defined and complex shallow reservoir system 3-7 ken indicates that the lava was not stored at shallow depths but rather beneath the surface. After passing through these filters, the lava can moved from its source region to the surface in short time periods only incorporate as xenoliths the wall rocks occurring at depths (Clague and Frey. 1982). shallower than the shallowest reservoir (dikes, sills, and olivine This analysis leads us back to Jackson's (1968) conclusion that cumulates} Alkalic lava of the postshield stage contains abundant only the xenoliths with metamorphic textures could possibly be xenoliths of dunite, which have CO2 inclusions that were trapped at mantle source rocks or residua. We conclude that only the lherzolite depths of at least 15 km, and cumulate xenoliths of rocks from and garnet peridotite xenoliths represent mantle rocks from below oceanic crustal layer 3 (Roedder, 1965; D.A Clague, unpub. the magma storage zone that appears to have existed beneath data, 1985). These observations suggest that in the postshield stage Hawaiian shield volcanoes at depths of 20-30 km. The dunite and any shallow magma chamber of the shield stage no longer exists but wehrlite xenoliths are either deformed cumulates formed during 26 VOLJ::ANISM IN HAWAII TABLE 1.8.-Distribution of Hcuxuion xenolith types [Data from Jackson (1968) except the alkalic preslueld stage which is from D.A. Clague (unpub. data, 198'»)] Xenolith type (percent) Dike rocks and Metamorphic Eruptive stage Lava type vein fi 11 iogs Cumulates rocks Alkalic alkalic basalt ( earlier stages in the volcano's growth or cumulates formed during 1983). The iron-rich olivine in all the xenoliths of this group led Sen formation of oceanic crust (see Sen, 1983, 1985; Kurz and others, (1983) to argue that they represent neither source rocks nor residua 1983; Sen and Presnall, 1985). related to Hawaiian lava. Frey (1980, 1984) has argued that they The remaining xenoliths of spinel lherzolite, rare harzburgite, may represent crystal accumulates from alkaline Hawaiian magma. and rare garnet peridotite that occur in alkalic lava of the rejuvenated We conclude that none of the xenoliths found in Hawaiian lava stage and even more rarely in alkalic lava of the preshield stage represent mantle source rocks or residua related to Hawaiian therefore are the only xenoliths of deeper mantle material. Spinel volcanism. They do, however, provide insight into the conduit lherzolite xenoliths have many characteristics that imply a dose systems through which much of this lava passed. genetic relationship to midocean-ridge basalt; however, both the Sr Jackson and Wright (1970) demonstrated Ihat xenoliths in the isotopic and rare-earth data indicate that these xenoliths have been Honolulu Volcanics were compositionally zoned in a geographic enriched by mixing between residua left after formation of midoceen sense with respect to the Koolau caldera; abundant dunite near the ridge basalt and an enriched magma or vapor (Frey 1980, 1984; caldera grades into lherzolite and finally garnet-bearing websterite Wright, 1984; Frey and Roden, in press). These xenoliths probably and pyroxenite away from the caldera. Jackson and Wright (1970) represent depleted oceanic lithosphere modified by processes related combined these observations with experimental petrologic and to Hawaiian magmatism. geophysical data to construct a cross section through the mantle and The final group of xenoliths consists of pyroxenite, websterite, crust beneath Oahu (fig. I. n Their cross section emphasizes the and garnet-bearing pyroxenite and websterite. These occur in only a mineralogic and compositional heterogeneity of the mantle beneath few vents of the alkalic rejuvenated stage in the Honolulu Volcanics Hawaiian volcanoes. However, the origins of many of the rock types (jackson and Wright, 1970) and on Kada Island (Garcia, Frey, are now thought to be different from those proposed by Jackson and and Grooms, in press). These rocks occur both as separate xenoliths Wright (I970~ A more recent model by Sen (1983) shows pla and as layers in xenoliths. Some of these xenoliths have been called gioclase lherzolite beneath the oceanic crust to a depth of about 30 garnet lherzolite (jackson and Wright, 1970), but they are not km (defined by the limit of plagioclase stability), spinel lherzolite merely a higher pressure assemblage of spinellherzolite because their from 30 to nearly 50 km, and garnet lherzolite below about 50 km. bulk compositions are distinct (jackson and Wright, 1970; Sen, The zone beneath the volcanoes includes cumulate dunite to depths I. THE HAWAIIAN·EMPEROR VOLCANIC CHAIN PART I 27 SALT LAKE Southwest Northeast CRATER KOOLAU CALDERA SEA LEVEL PACIFIC OCEAN 0"," o _.. sw 1/ ....___--.. :}A~f~~~~"CE'[~i~jf •... L ....- fflj~kt~H;~l~i;;"i BASALT ANO·· "" . "'. '. "."'-- SERPENTINITEl?) OCEANiC CRUST PLAGIOCLASE 20 '5 LHERZOLITE EANJ DUNITE AND HIGH-VELOCITY MANTLE PLAGIOCLASE Kootau OLIVINE-RICH (P ~ 8.0 kml ) LHERZOLITE a: magma PERIDOTITE '"w 30 chamber >-w Nephelinite-+- 40 :; feeder SPINEL 0 dikes SPINEL LHERZOLITE ~ LHERZOLITE ;Z Oikes 45 ;; Garnet- feeding bearing Koolau , I' pyroxenite magma , 60 >- sulle chamber 0. , - Zone w , , 0 60 ) , , °illh"" lOW-VELOCITY ~ DUNITE ~ MANTLE WYf-~\\IrtX GARNET 11111 .I LHERZOLITE tholeiite (P < 8.0 kml ) 80 11111 I 75 GARNET HARZBURGITEln meltin 1\' I ..• «0 0 5 10 KILOMETERS 'DO GARNET; MINIMUM'.;.c 'pYROXENITE' " _--~ ,VELO~ITY ._.AND ".' b ...--d' FIGURE 1.IO.-Cross section beneath Oahu from Sen (1983) showing configura ,LHERZOLITE 'Z- ,. ZONE Zone of Honolulu , tion of various mantle source and residual rocks brought to surface as xenoliths of ,.. , ...' Volcanics rnettinn abundant dunite, lherzolite, and garnet peridotite by rejuvenated-stage Honolulu o 20 KILOMETERS Volcanics. I FIGURE 1.9.-Cr055 section beneath Oahu from Jackson and Wright (1970~ Dunite zone inferred to be mantle residue left behind from partial melting thai forms Koolau tholeiitic shield lava. Configuration of rock types and their mode of chemically and mineralogically similar to alkalic rejuvenated-stage origin are far different from those shown in figure 1.10. lava from the Hawaiian Islands (table 1.2). The identification of which dredged or drilled lava samples erupted during which eruptive stage relies on comparison of the major-element compositions to those of the various Hawaiian lava types (table 1.7) in conjunction of about 15 km (fig. I. 10). The areal distribution of xenoliths with trace-element ratios (Clague and Beeson, 1980; Clague and observed by Jackson and Wright (1970) reflects passage of the others, 1980c, Frey and Clague, 1983) and mineral compositions Honolulu Volcanics lava through the zone of dunite cumulates. (Keil and others, 1972, Fodor and others, 1975, Clague and others, I980a). In particular, we have found that the composition of groundmass pyroxene and the K/Ba and PzOs/Zr ratios seem to PETROLOGY OF LAVAS ALONG THE VOLCANIC CHAIN separate alkalic basalt of the postshield and rejuvenated stages. In the middle to late 1970's new studies added data to the Rejuvenated-stage alkalic basalt has lower KlBa and higher already complex data array on Hawaiian volcanoes. Studies on lava PzOs/Zr ratios and pyroxene with more calcic compositions and recovered from the older submarine portions of the chain (Clague, higher concentrations of N a, 11, and AI than postshield-stage 1974, Dalrymple and others, 1974, 1977, 1981, Clague and alkalic basalt. Lava samples recovered from the volcanoes west of others, 1975; Dalrymple and Clague, 1976, Kirkpatrick and the principal Hawaiian Islands are discussed in appendix 1.1 and others, 1980, Clague and Frey, 1980, Lanphere and others, 1980, summarized in table 1.9. Dalrymple and Garcia, 1980; Garcia, Grooms, and Naughton, in Several conclusions may be drawn from these studies of press) clearly demonstrate that the volcanoes of the entire Hawaiian samples from along the Hawaiian-Emperor Chain. The first con Emperor volcanic chain erupted tholeiitic basalt and picritic clusion is that the Hawaiian hot spot has produced very similar lava tholeiitic basalt similar to those of the shield stage in the Hawaiian types in the same eruptive sequence for at least the last 65 m.y. Islands. In addition, alkalic lava similar to that erupted during the (table 1.\0). Samples from the same eruptive stage are similar to one postshield stage in the Hawaiian Islands, including hawaiite, another in both major- and trace-element compositions, including mugearite and trachyte, is commonly recovered from the older rare-earth elements (Clague and Frey, 1980, Frey and Roden, in volcanoes. In the drill holes on Ojin and Suiko, tholeiitic lava occurs press), Isotopic studies indicate, however, that small systematic below alkalic lava, as in the Hawaiian Islands. Some samples are changes occur over time (Lanphere and others, 1980; Unruh and 28 VOLCANISM IN HAWAII TABLE I .9.-Rock IYPC5 and inferred volcanic 5{ages represented along the Hawaiian-Emperor Chain [X, present; __• not present or not known; (T), transitional; volcano numbers from Bargar and }acbon (1974)] Shield stage Alkalic postshield stage Alkalic re juvenated stage ~ ~ •" .0" ."o ~ ~ ~ .- ." ~ •" " ~ .:: .0" 0 " u ~ • "• ~ ~ " "' ~ .0" " .0 ." ~ .-u u " ." u u " C " u " ~ " ." .-u u " u ~ u ." " ~ .-." u • ." .-u e-, .- .~ ."" .- " -c .- "u ." c ~ c ."~ u" Volcano ~ .-u "0 "'c e .c 0 u >- " , " 0 "c,.- c, Number Name "c " "0 u .a " "• "' ."c, @ -e " • "" " c, ;;;" "'..... " -e '" " .... '"" z" "" ...." 1 Kilauea ------X X 2 Mauna Loa ------X X 4 Hualalai ------XX X X X 3 Mauna Kea ------X K X X X 5 Kohala ------X XX 6 Haleakala ------X X X X X XX 7 Kahoolowe ------X X X X, 8 West Maul ------X X XXX X X 10 East Molokai ------XX X X X XX XX 9 Lanai ------XX 11 West Molokai ------X X X X 12 Koolau ------X X X X XX 13 Waianae ------X X X X 14 Kauai ------X X X XXXX 15 Niihau ------X X X X 15A Kaula ------X X X 17 Nihoa ------X X 19 Unnamed Seamount X 20 Unnamed Seamount ------X X 21 Unnamed Seamount ------X 23 Necker ------X X, X X, 26 La Pe r o use Pinnacles -- X 30 Gardner Pinnacles ----- X X 38 Brooks Bank ------X X 29 St. Rogatein Bank ----- X 36 Laysan ------XX 37 Northampton Bank ------X X 39 Pioneer Bank ------X 50 Pearl and Hermes Reef - XX X 51 Ladd Bank ------X 52 Midway Is land ------X X X 53 Nero Bank ------X 57 Unnamed Seamount X 63 Unnamed Seamount ------IX 65 Colahan Seamount ------( T) IX 65A Abbott Seamount ------( T) 67 Daikakiyi Seamount ---- X X 69 Yuryaku Seamount ------X 72 Kil1Ullei Seamount ------X 74 Koko Seamount (southeast) ------X XXXX X 76 Koko Seamount (northwest) ------X 81 OJ in Seamount ------X X 89 Jingu Seamount ------X X 86 Nintoku Seamount ------X 90 Su i ko Seamount (southern) ------X, 91 Su.i ko Seamount (central) ------X X X 108 Meiji Seamount ------X IDredges from unnamed seamount (63) and Calahan Seamount recovered ankaramite, tephrite, and amphibole-bearing hawaiite that a TAIIl.E I. ID.-Composition of tholeiitic basah from iJo{cunocs of the Heuciion-Emperor Chain rAil figures in wtiKht percent. dry Tl'duCl'd norm..heed average atlilly~eJ; olivilll"added or subtrected so thaI Mg/(Mg+O.8S Fe) =-0.70: __ , not analyzed: PI0,; value in parentheses is high due to marine Vhosplhltililtiofll Volcano Ki l auea Mauna Hauna HuaLal.ai Koh a l a East West Lana l East West Koolau Waianae Loa Kea M Si02 -- 48.9 50.5 46.4 49.4 48.2 49.7 47.J 49.0 46.4 49.2 51. 5 46.9 47.9 A1ZO) - 12.1 12.2 12.8 1\.8 J).5 13. ) 12.6 12.8 12.9 II .8 13 .2 13.4 14.1 reO --- 11.4 11.0 12.3 II .9 11.8 10.9 12.2 11.0 12.4 11. 9 10.4 11. 9 11. 2 MgO --- 12. 7 12.J 1].6 13.4 IJ .1 12.1 1).7 12.3 13.8 13 .2 It. 7 13.2 12.5 CaD --- 9.7 9.2 9.9 U 9.4 9.6 9.' 8.8 9.7 '.9 '.3 9.1 9.6 NaZO -- J. 99 I. 98 I. 82 I. 84 1. 62 1.76 1.66 2..13 1. 89 2.42 2.47 2. 07 1.86 K:;O --- .44 .36 .28 .23 .10 .33 .23 .11 .20 .18 .27 .53 .26 TtOz -- 2.34 1. 85 2.40 1. 75 I. 93 2.01 2. 14 1. 66 2.22 2.08 I. 68 2.46 2.20 PZOS -- .22 .21 .23 .16 .20 .13 .20 .18 .25 .22 .35 .25 MnO --- .17 .16 .17 .15 .18 .18 .17 .14 .18 .19 .15 .15 .17 Volcano Kauai Ni i hau Nihoa Unnamed Unnamed Necker- L, Pe r o use Gardner Northampton Pioneer Daikakiji Su i.k o (20) (21 ) Island pinnacles Pinnacles Rank high riOZ low TiOZ Si02 -- 48.4 48.4 47.4 46.9 47.1 47.15 47.5 47.6 48.7 48.2 49.7 47.6 47.9 AIZO) - 12.5 12.1 11.5 11.2 1t.) 11.1 11. 7 12.5 11.4 11.2 11.5 12.7 13 .0 FeD --- 11.9 12.1 12.4 12.6 12.4 12 .8 11.8 II.J 11. 7 It. 9 II .5 12.3 11.9 MgO --- 13.3 13.6 13.8 14.0 13.8 14.1 13 .1 12.6 13.0 13.3 12.9 13.7 13.2 CaD --- 9.2 8.1 9.4 9.6 9.2 9.8 10.7 10.J 10.1 9.8 9.05 8.7 9.3 NaZO -- I.93 2.28 1. 77 2.06 2.25 I. 59 1. 82 2.06 2.00 2.20 1.08 2.26 2.26 K:;O --- .30 .49 .26 .24 .64 .38 .39 .16 .32 .67 .43 .28 .14 nuZ -- 2.06 2.49 2.59 2.97 2.72 2.47 2.44 I. 98 2.26 2.36 2.32 2.10 I. 86 F20) -- .23 .3I ( .70) .28 .35 .36 .34 .26 .23 .17 .36 .22 .16 HnO --~ .17 .16 .15 .15 .15 .17 .20 .16 .16 .14 .16 .18 .18 others, 1983). The lower 87Sr/86Sr ratios and higher 143Nd/ 144Nd lower 143/Nd 144Nd and Rb/Sr raIios than the later alkalic lava ratios of lava from the central Emperor Seamounts compared to from the postshield and rejuvenated stages. They proposed a those of lava from the Hawaiian Islands and Ridge imply that complex mixing model to explain the apparent paradox of having tholeiitic lava erupted 65 m.y, ago was derived from a more depleted more radiogenic isotopic ratios combined with more depleted trace source than that erupting today. Lanphere and others (1980) element ratios in the same rocks. Their model proposes two sources, correlated this observation with the data shown in figure 1.3 to a primitive mantle-plume source and a depleted oceanic-lithosphere suggest that the chemistry of Hawaiian tholeiitic lava has varied as a source, which can mix before melting or can produce partial melts function of the age and thickness of the oceanic lithosphere beneath which then mix. They argue that small amounts of small-percentage each volcano when it was constructed. The correlation suggests that melts from the oceanic lithosphere (midocean-ridge source) are the oceanic lithosphere forms at least part of the source material for mixed with enriched mantle or with melts derived from enriched Hawaiian tholeiitic magma, or that the magma partially reequili mantle. This model is similar to earlier selective-melting models bretes with the oceanic lithosphere. Wright (1984) proposes that qualitatively proposed by Green and Ringwood (1967) and Mac Hawaiian magma originates from oceanic lithosphere converted to donald (1968). It would also be possible to mix small-percentage asthenosphere. melts of enriched mantle with the oceanic-lithosphere source (basically an enrichment model) to create the source rocks for Hawaiian magma (Clague and others, 1983; Chen and Frey, STRATIGRAPHIC STUDIES IN THE HAWAIIAN ISLANDS 1985\ although the measured and calculated compositions do not Studies of stratigraphically controlled samples (Beeson. 1976; match as closely as in the model of Chen and Frey (1983) All these Clague and Beeson. 1980; Chen and Frey, 1983; Clague and models predict a range of source compositions from which the lava is others. 1983; Feigenson, 1984; Lanphere and Frey, 1985) have generated. shown that major-element, trace-element, and isotopic ratios change Other studies emphasize the bulk composition of the source systematically as a function of time at some Hawaiian volcanoes. rocks and the processes and physical conditions of the melting These observations are not universal (Stille and others, 1983 ; Frey process. For example, Clague and Frey (1982), from a deIailed and others, 1984) in as much as Waianae and Mauna Kea erupted trace-element analysis of the rejuvenated stage Honolulu Volcanics isotopically similar lava during the tholeiitic shield and alkalic on Oahu, concluded that lava ranging from nepheline melilitite to postshield stages. Chen and Frey (1983) observed systematic alkalic basalt was generated by 2-11 percent partial melting of a stratigraphic trends in 8'Sr/86Sr, Rb/Sr, 143Nd/ 144Nd, and Smi homogeneous garnet « I0 percent) lherzolite source that was carbon Nd ratios in samples from East Maui Volcano. Their data indicate bearing. The source had been recently enriched and had a that the tholeiitic lava had higher /j7Sr//j6Sr and Sm/Nd ratios and chondrite-normalized La/Yb ratio of 4.4. During melting, phlo- 30 VOLCANISM IN HAWAII gopite, amphibole, and a Ti-nch phase (oxide?) remained in the Craig, 1983; Kaneoka and others, 1983). The ratio of 'He/4He is residua, but apatite was completely melted. This model can be inversely related to the volume of the volcanoes on the Island ol combined with the model of Chen and Frey (1983) to generate the Hawaii (Kaneoka. chapler 27; Kurz and others, 1983), suggesting source composition indicated for the Honolulu Volcanics (see Roden that at smaller volcanoes lava is generated from sources that art and others, 1984). The homogeneous composition of the mantle largely primitive and not degassed. Another observation is thai source for the Honolulu Volcanics implies that the recent enrichment Hawaiian volcanoes initially erupt alkalic lava generated from event affects a large volume of depleted mantle from which the lava is heterogeneous source compositions by rather small percentages 01 then generated by partial melting. This is not the same process partial melting (Moore and others, 1982; Frey and Clague, 1983). espoused in the model preferred by Chen and Frey (1983) in which The evolutionary sequence at a Hawaiian volcano is therefore from enriched mantle or partial melts of enriched mantle mix with partial small-volume, infrequent eruptions of small-percentage melts to melts of depleted mantle. Note that all these models consider only large-volume, frequent eruptions of large-percentage melts, and then two mixing end members, whereas the isotopic data clearly indicate back to small-volume, infrequent eruptions of small-percentage melts that at least three distinct source compositions are required (Tat (Wise, 1982). sumcto, 1978; Staudigel and others, 1984). Feigenson (1984) proposed three-end-member mixing models for Kauai lava but did PETROLOGIC OVERVIEW not identify the trace-element signatures of the source components. The generation of large volumes of tholeiitic lava has been the In summary, the petrology of lava from along the Hawaiian focus of recent studies by Wright (1984) and Budahn and Schmitt Emperor Chain indicates that at least three source materials are (1984), who used different approaches and reached dramatically involved in the generation of Hawaiian lava; one of these sources is different conclusions. Wright (1984) used mess-balance considera apparently the depleted ocean lithosphere, whereas another is tions to calculate the components and abundance of material that relatively primitive undegassed mantle. The third component is less must be added to depleted lithosphere to generate Hawaiian well defined. Since multiple sources are required, mixing of these tholeiitic basalt by large percentages of partial melting (35-42 sources or of melts generated from these sources must occur. The percent melting). His models did not attempt to calculate the compositions of lava along the chain apparently are related to the age variations in source composition for tholeiitic basalt from the dif (thickness) of the underlying oceanic lithosphere; the volcanoes ferent volcanoes (Leeman and others, 1977, 1980; Basaltic Vol formed on younger and thinner oceanic lithosphere were generated canism Study Project, 1981). Budahn and Schmitt (1984) used from a source with a larger component of the depleted ocean inverse procedures to estimate the variations in source composition lithosphere. Detailed overviews of the petrology of Hawaiian required to generate the tholeiitic basalt from a number of Hawaiian tholeiitic lava and Hawaiian alkalic lava are presented in Wright and volcanoes. Their estimated sources had 74-86 percent olivine plus Helz (chapter 23) and Clague (in press), respectively. orthopyroxene, 11-21 percent clinopyroxene, and 3-5 percent Volcano volume reflects the degree of melting of the tholeiitic garnet. All the calculated sources had slightly enriched light-rare basalt and probably also the size and frequency of intrusion of earth-element contents, and low heavy-rare-earth abundances (0.9 magma batches. The inverse correlation of volcano volume with 4 to 1.6 limes chondrites). They calculated the partialmelting at 2-10 3 He/ He ratio in tholeiitic basalt indicates that smaller percentage percent for these sources. Budahn and Schmitt (1984) did not melts are derived from sources with more of the primitive component address the processes that led to creation of these different source and larger percentage melts are derived from sources with less of the compositions, nor did they consider the volumes of mantle source primitive component. Volcano volumes and compositions of the regions required, or the constraints on the production of partial melts shield tholeiitic basalt are also related, less-enriched tholeiitic basalt provided by Kilauea's magma supply and eruption processes. forms larger shields and more-enriched tholeiitic basalt forms smaller Wright's (1984) model follows from consideration of these additional shields (Clague and Frey 1979), although this correlation is imper constraints. The large difference between the models of Wright fect. Models developed in the future should address the problem of (1984) and Budahn and Schmitt (1984) emphasizes the uncertain characterizing the isotopic and trace-element compositions of the ties concerning the compositions and processes that create the source three mantle components and address the timing and processes of rocks and the lava of the Hawaiian Islands. mixing of these sources. The source volumes inferred from different melting models must he considered. Wright's (1984) model requires only modest source volumes, whereas the model of Budahn and PETROLOGIC STUDIES OF LOIHI SEAMOUNT Schmitt (1984) requires partial melting of a mantle zone 100 km Studies of Loihi Seamount have provided new insight In thick and 100 km wide to generate the volcanoes of the principal magma genesis in the Hawaiian Islands. Trace-element and isotopic Hawaiian Islands. Such enormous inferred volumes of mantle source studies demonstrate that the source rocks beneath a single volcano rock pose numerous problems for models advocating small-percen are heterogeneous and require at least three mantle components tage melting to generate the tholeiitic shields. (Frey and Clague, 1983; Lanphere, 1983; Staudigel and others, A separate problem is the cause of the alkalic rejuvenated 1984). Perhaps more important is the observation of very high stage. Jackson and Wright (1970) used tide-gage data from Moore 3Hel4He ratios, which imply a primitive undegassed source of (1970) to suggest that generation of the rejuvenated-stage Honolulu volatiles (Kaneoka, chapter 27; Kurz and others, 1983; Rison and Volcanics might be caused by uplift as Oahu has passed over the I. THE HAWAIIAN·EMPEROR VOLCANIC CHAIN PART I 31 Hawaiian Arch. They argued that the Hawaiian Arch, an isostatic and paleomagnetic and other data that Morgan's hypothesis of response to volcanic loading on the oceanic crust, follows the relative hot-spot fixity is basically correct, but that the fixity of the progression of active volcanic centers by several hundred kilometers hot-spot frame of reference with respect to the spin axis, particularly and several million years. Clague and others (1982) showed that the in early Cenozoic and Late Cretaceous times, is not established. duration of the quiescent period preceding eruption of the rejuve nated-stage lava has decreased systematically from nearly 2.5 m.y. on Niihau 10 <0.4 m.y. at Haleakala (see fig. 1.6). They suggested PALEOMAGNET'C TESTS OF HOT·SPOT FIXITY that a new mechanism should be sought to explain the age data. We have reexamined the data and conclude that they are consistent with Age data along the chain have shown that there has been more the model proposed by jackson and Wright (1970) because the rate or less continuous relative motion between the Hawaiian hot spot and of volcanic migration is increasing. The rejuvenated stage follows the the Pacific plate, thereby proving the kinematic aspect of the hot formation of the shield not by a constant time but by a constant spot hypothesis, but these data have little or no bearing on the distance. The rejuvenated-stage Koloa Volcanics on Kauai and question of hot-spot fixity. The lava flows that form volcanoes of the Kiekie Basalt on Niihau began erupting during formation of the Hawaiian-Emperor Chain, however, contain a nearly continuous Koolau shield located 180-225 km to the southeast. Likewise, the magnetic record of the latitude of the Hawaiian hot spot for the Honolulu Volcanics on the Koolau Range of Oahu began erupting entire Cenozoic and the latest Cretaceous. Although only a small during formation of the East M aui shield located 160 km 10 the fraction of this magnetic record has been read, there are now southeast. The rejuvenated-stage Kalaupapa Volcanics on East sufficient data to provide a partial test of the fixity hypothesis for the Molokai erupted during formation of the Mauna Kea shield located Hawaiian hot spot. Paleomagnetic data from volcanoes along the 200 km to the southeast. Finally, the rejuvenated-stage Hana chain show that the Hawaiian hot spot (and thus presumably the Volcanics on East Maui began erupting during formation of the worldwide hot-spot frame) has been, to a first approximation, fixed Mauna Loa shield, located 160 km to the southeast. In each case, with respect to the spin axis since the time of formation of the the lava of the rejuvenated stage began erupting during formation of Hawaiian-Emperor bend. The limited data indicate, however, that a large shield 190 ± 30 km to the southeast. The Hawaiian Arch is there was motion between the hot spot and the spin axis, that is, true aboul 250 km from the center of the volcanic ridge, bUI only 210 km polar wander, before that time. to the east-southeast of Hawaii (Walcott, 1970). It is therefore likely The paleolatitudes of several Hawaiian-Emperor volcanoes, as that a factor in magma generation during the rejuvenated stage is the determined from paleomagnetic studies on individual rock samples rapid change from subsidence to uplift as the volcanoes override the and from shipboard magnetic surveys, are given in table 1. 11 and flexural arch created by formation of large shields. To the northwest plotted in figure 1. 11 as a function of volcano age. In general, the of the Hawaiian Islands the rates of volcanic propagation were data indicate that the Hawaiian-Emperor volcanoes formed not at slower and more constant; we predict that lava of the rejuvenated their present latitudes but at a latitude near the present latitude of stage will postdate the shield stage by 2-3 m.y. We also suggest that Hawaii. Thus, the latitude of the Hawaiian hot spot has been the apparent paucity of lava from the rejuvenated stage to the approximately fixed throughout the Cenozoic. The data are not of northwest of the Hawaiian Islands may reflect the absence of large uniform quality, however, and some care must be exercised in their volcanic edifices capable of flexing the lithosphere sufficiently. Like interpretation. wise, the absence of any lava samples of the rejuvenated stage from The paleomagnetic data have been discussed and evaluated by the Emperor Seamounts may result from the rather wide spacing Jackson and others (1980), Kono (1980), and Sager (1984), who between volcanic edifices: by the time the next younger volcano point out that the paleomagnetic sampling of Mejji, Nintoku, Ojin, formed, the previously constructed volcano was already beyond the Midway, Nihoa, and the Island of Hawaii involved a small number arch. The fact that the Emperor volcanoes were constructed on of lava Bows, making it doubtful that the secular variation is young, thin lithosphere would amplify this effect because the dis adequately averaged out. The errors for the Ojin and Nintoku sites tance from the load to the Rexural arch decreases as the lithosphere reflect this uncertainty, but there is reason to suspect that the errors becomes less rigid. assigned to the paleolatitudes of Midway, Meiji, and Nihoa are too small. This is because of the unusually low dispersions and the FIXITY OF THE HAWAIIAN HOT SPOT likelihood of serial correlation of some of the flows, which further decreases the number of independent measurements from the sites. Wilson's original hypothesis for the origin of the Hawaiian and The paleolatitude of 17.5°±5°, determined for Suiko by other island chains by passage of the crust over a source of lava in the Kodama and others (1978) from magnetic survey data, is suspect mantle (Wilson, 1963a, b, c) did not require that the hot spot be for several reasons. First, the magnetic anomaly over Suiko is fixed, only that it have some motion relative to the crust above it. complex, resulting in a low statistical test of fit (R = 1.1) for the Morgan (1972a, b), on the other hand, specified that a worldwide inversion. Second, it is likely that Suiko is constructed from several system of thermal plumes (hot spots) was fixed in the mantle and that coalesced volcanoes (Bargar and Jackson, 1974), possibly of dif the relative movement between them was small or negligible. Several ferent ages, and the necessary assumption of uniform magnetization workers (for example, Minster and others, 1974; Gordon and is probably invalid for this seamount. In addition, the paleolatitude Cape, 1981; Morgan, 1981) have shown from relative plate motions is inconsistent with that obtained from the paleomagnetic study of 32 VOLCANISM IN HAWAII TABLE I.II.-Paleolatiludcs dclcnnincd for volcanoes 0/ the HauJaiian-Empcror still a minimum of 40 independent data. There are also 12 places in Chain the cores where the inclination changes by more than 15°, which [From paleomagnetic mea,uremenls on lava flows and from shipboard magnetic ,urvey' (SM~ indicates that at least 13 secular variation cycles have been sampled, Data from compilation, by Kono (1980) and Sager (1984); the more reliable data (Sager, 1984) underlmed; uncertainties aTI' Ihe values of o.9~J making it likely that secular variation has been adequately averaged out. Other paleomagnetic stability indices indicate that 27.lo±3.5° N"mber ,f Present Paleolatitude is a highly reliable measure of the latitude of formation of Suiko VOleano flows latitude { degrees Seamount (Keno, 1980). Number Name determined ( degrees north) north) 1,2,4, Kilauea, Mauna L" 17 19.5 19.5*1.4 Hua La lai (historical) 1,2.3 Kilauea, Mauna Loo 8 19.5 17.HIO.7 BIOfACIES AND TEMPERATURE DATA fROM THE Mauna Kea( 14 C dated} HAWAIIAN·EMPEROR CHAIN 12 Koolau JJ 21.4 16.8i).6 13 Waianae 55 2J.S 15.H3.3 14 Kauai. (Maka",e!i Member I Although northward displacement of the Hawaiian hot spot Waimea Canyon Basalt) 25 22.0 15.6±3.1 relative to the spin axis is only indicated by the single paleolatitude 14 Kauai (Napali Member. \oIaimea Canyon Basalt) 46 22.1 14.9%3.1 from Suiko, it is supported by a variety of additional data. Analysis 17 Ni hoa 14 23.1 21.0%6.6 52 Midway 13 28.2 15.4%5.4 of Pacific deep-sea sediment cores, for example, shows that the 65A Abbott (SM) 31.8 17.5:12.4 81 OJ in 6 38.0 ~2 paleoequator was 10°-16° farther north than at present between 86 Nintoku 4 41.3 36.0:1:.24.6 about 75 Ma and 65 Ma (Sager, 1984). 91 Suiko { SM) 44.8 16.7±S 91 Suiko 65 44.8 27.1%3.5 Biofacies data from DSDP Leg 55 drilling in the Emperor 108 Heij i 6 53.0 19.2%4.1 Seamounts provide semiquantitative substantiation of the Suiko paleolatitude. The bioclastic sediment on Suiko, Nintoku, and Ojin Seamounts consists primarily of coralline algae and bryozoans with ostracodes, foraminifers, and assorted shell fragments typical of a Suiko (Kono. 1980), which is the best study of its kind for any of the shallow-water, high-energy environmenl (jackson and others, 1980). volcanoes in the chain. Only a single coral was found in the Suiko material, and none was Sager (1984) included in his compilation Iwo additional deter recovered from either Ojin or Nintoku, indicating that corals were minations from the principal Hawaiian Islands that we have chosen not significant contributors to the carbonate buildups. to omit from table I. II. These include a group of 129 flows from the Schlanger and Konishi (1975) have pointed out that carbonate Islands of Hawaii and Niihau, and a second group of 19 flows from buildups in the Pacific can be divided into bryozoan-algal and coral Kauai. Both groups include flows from the rejuvenated stage that algal facies, the distribution of which depends largely on water were erupted several million years after the hot spot had moved temperature and solar insolation and thus is, to a large degree, a (relatively) southeastward 10 form new tholeiitic shields. Although function of latitude. They observe that in the modern Pacific, the both of these determinations were included by Sager in his list of coral-algal facies dominates at latitudes less than about 20°, whereas more reliable paleolatitudes, they are so close to the present position the bryozoan-algal facies is predominant above about 30° latitude. of the hot spot that their elimination has no significant impact on the They locate the boundary between these facies at about 25° latitude, conclusions drawn from the data. but emphasize that the transition is gradual. In the central Pacific, Taken at face value, the more reliable paleolatitude data (fig. the annual surface-water temperature at 25 0 latitude is about 22°C I. II) indicate that the Hawaiian hot spot may have been a few (Muromtsev, 1958), which is usually considered the minimum for degrees south of its present position during the late Cenozoic, near its active coral-algal reef growth (Vaughn and Wells, 1943; Heckel, present position when Abbott Seamount formed at about 39 Ma, 1974). The optimum temperature for vigorous reef growth is 25-29 and r north of its present position at Suiko time, 65 Ma. Analyses °C. Thus, the existenceof carbonate buildups of the bryozoan-algal of paleoequator (Sager, 1984) and worldwide paleomagnetic data facies atop Ojin, Nintoku, and Suiko Seamounts indicates that the (Livermore and others, 1983), however, show that there has been reefs atop the volcanoes formed in water temperatures less than little or no motion of the spin axis relative to the worldwide hot-spot about 22 'c. frame during the past 40 m.y. or so. From this comparison of Using the oxygen-isotope temperature data of Savin and others independent data Sager (1984) concluded Ihat the apparent south (1975) for the North Pacific, Gfeene and others (1978) recon ward displacement of the Hawaiian hot spot shown by the data from structed the approximate latitude variation through time for the 20 younger volcanoes in the chain (fig. 1. II) reflected changes in the 'C and 22 'C isotherms (fig. 1.12). They showed that if the magnetic field rather than relative movement between the hot spot Hawaiian hot spot were fixed, then Suiko Seamount would have and the spin axis. formed in water warm enough to have developed active coral-algal The apparent displacement indicated by the Suiko data, reefs. Following the analysis of Greene and others (1978), Jackson however, is probably real. The Suiko paleolatitude is based on and others (1980) showed that the Paleocene water temperature at analysis of a large number of flows (table I. II) recovered by coring the latitude determined by the paleomagnetic data from Suiko was over an interval of 550 m (Kana, 1980). Even when certain flows appropriate for the bryozoan-algal carbonates that occur imme thought to represent a very short time interval are grouped, there are diately above the basalt. o I I I I I o 10 20 30 40 50 60 70 POTASSIUM-ARGON AGE IMal FIGURE 1.11.-Paleolatitude plotted against age for volcanoes along Hawaiian-Emperor Chain. Crosses, present latitude. dots and circles, paleolatitudes determined from paleomagnetic data; triangles, paleolatitudes determined from shipboard magnetic surveys. More reliable data indicated by solid symbols. Error bars show O:9~' Dashed reference line is backtracked position of hot spot relative 10 Pacific plate assuming a constant velocity of 8 em/yr. Paleomagnetic data from table 1. , 1, age data from table 1.4 and appendix 1.1. The paucity of coral material on seamounts in the central time Abbott Seamount formed just after formation of the Hawaiian Emperor Chain is in contrast to Koko and the seamounts on the Emperor bend; the slightly cooler temperatures indicated by the bend, where corals are more common but still less abundant than in carbonate facies and temperature data from the bend seamounts are a region of vigorous coral reef growth (Davies and others, 1971, probably related to the sudden drop in ocean temperature in the late 1972; Matter and Gardner, 1975). Oxygen-isotope temperatures of Eocene rather than to a more northerly hot spot. carbonate diagenesis for Suiko, Nintoku, Oim, and Kammu Sea Thus, the paleomagnetic data from Suiko, the biofacies and mounts (McKenzie and others, 1980) show a gradual warming from temperature data from the central and southern Emperor Sea Suiko to Koko, at least in part caused by southward migration of the mounts, and the Pacific paleoequator data all indicate southward hot spot (jackson and others, 1980). Thus, the biofacies and migration of the Hawaiian hot spot in the early Tertiary and Late paleotemperature data from Leg SS are consistent with the pal Cretaceous. This conclusion is consistent with previous findings, eomagnetic data, indicating a latitude of 27° for the hot spot at Suiko based on analysis of worldwide paleomagnetic data in the hot-spot time. The data are also consistent with Sager's (1984) suggestion frame of reference, of about 10° of southward movement of the hot that the hot spot had reached its approximate present latitude by the spot frame relative to the spin axis (that is, true polar wander) 34 VOLCANISM IN HAWAII 50 ,-~--~-~~_~__-,-_~__-, have attempted such evaluations for the Pacific plate since Morgan (1971) first proposed the technique. Most of the linear volcanic I chains in the Pacific basin are oriented roughly west-northwest and ~ 40 a apparently formed sequentially over nearly stationary hot spots z , during the last 43 m.y, as the Pacific plate rotated clockwise about a '"w ~ 30 : pole located near lat 69' N., long 68' W. (Clague and Jarrard, o ,,, w , , ,-, 1973). Another group of linear chains exhibit roughly north-trending a , , ,, ,, ~ \\'" , , orientations and apparently formed by the same mechanism between HOT-SPOT PATH ui .r ,\ a , at least 80 Ma and 43 Ma as the Pacific plate rotated clockwise ::> " about a pole located near lat 17' N., long 107' W. (Clague and f ",',, «i= , , Jarrard, 1973). ~ , , ~6 The hot spots that formed the Hawaiian, Austral-Cook, ~~ Society, Marquesas, Caroline, Pitcairn-Gambier. Samoan, and , ' Islas RevillaGigedos islandchains and the Pratt-Welker and Cobb MIOCENE OUGOCENE EOCENE PALEOCENE I-- LATE MID EARLY LATE EARLY LATE MIDDLE UAlY lATE URlY 5 Eickelberg seamount chains moved very little with respect to one a 10 20 30 40 50 60 70 another (Duncan and Clague, 1985). The most convincing evidence AGE, IN MILLION YEARS that hot spots move with respect to one another comes from the orientation of the Marquesas Islands, which is discordant by about FIGURE 1.12.~Approximateposition of 20°C and 22 °C surface-water isotherms 25° with that predicted, implying motion of the Marquesas hot spot in north-central Pacificduring Cenozoic, modified from Greene and others (1978), to the northeast with respect to the hot-spot reference frame at based on data of Savin and others (1975). Dots, paleolatitudes of Suika Seamount assumingthat Suiko formedal 27° N. and that hot spot has been fixed sincelimeof several centimeters per year (jarrard and Clague, 1977) during the bend formation. Circles, paleolatitudes for Suiko assuming a fixed hot spot for past last 5 m.y. The rates of volcanic migration along the chains younger 65 m.y. Squares, positions of formation of Koko Seamount and bend under same than 43 Ma fit a pole of rotation at lat 68' N., long 75' W. and an assumptions. Backtracking was about an Emperor pole at lat 17° N .• long lor angular rotation rate of 0.95°±0.02°/m.y. (Duncan and Clague, W. and a Hawaiian pole at lat 69° N .• long 68° W. (Clague and Jarrard. 1973). 1985). The 22°C isotherm is approximate boundary between coral-algal (warmer) and bryozoan-algal (colder) facies of Schlanger and Konishi (1975). CAUSE OF THE HAWAIIAN-EMPEROR BEND An especially knotty problem over the past decade has been the relationship between Pacific sea-Roar spreading, worldwide plate motion, and the Hawaiian-Emperor bend. Since there is now firm evidence that the motion of the hot-spot frame was small during during the latest Cretaceous and earliest Tertiary (for example, the early Cenozoic and has been negligible since then, the 120° angle Gordon and Cape, 1981; jurdy, 1981, 1983; Morgan, 1981; in the Hawaiian-Emperor bend must represent a major (circa 60°) Gordon, 1982). change in the absolute motion of the Pacific plate. Since the motions The paleolatitude of 17.5'±4.4' N. found for Abbott Sea of individual plates are not independent, we would expect such a mounl puts the Hawaiian hot spot at about its present latitude by 40 significant change to be part of a worldwide reorganization of both Ma, which is consistent with the conclusion of Livermore and others absolute and relative plate motions. Various authors have suggested (1983) that true polar wander did not occur during the past 35 m.y, that the bend might correlate with circum-Pacific tectonic events The paleoequator analysis of Sager (1984) suggests that there was (Jackson and others. 1972; Clague and Jarrard. 1973; Moore, no true polar wander after formation of the bend. that is, after 43 1984), that it may be caused by the collision of India and Eurasia Ma. This requires approximately 7.6° of southward latitudinal (Dalrymple and Clague, 1976), or that it may be the result of new motion of the hot spot between 65 Ma and 43 Ma and 5° of subduction zones along the southwestern margin of the Pacific plate northward motion of the Pacific plate in order to satisfy the relative (Gordon and others, 1978~ However, completely satisfactory cor motion of about 0.65° latitude per million years indicated by the relations have not been achieved. age-distance data. A major feature of the northeast Pacific magnetic-anomaly pattern is the major change in the trend of the magnetic anomalies, that is, the magnetic bight. between anomalies 24 and 21. Recon COMPARISON TO OTHER PACIFIC LINEAR ISLAND CHAINS struction of the Pacific plate shows that this change in the anomaly Another way of evaluating the movement of hot spots is to pattern is the result of a change in spreading about the Pacific-Kula compare the orientation and age progression quantitatively along Farallon triple junction, in particular the cessation of spreading on volcanic chains formed during the same time period on the same the Kula Ridge (Scientific Party DSDP 55, 1978; Byrne, 1979). plate. Several studies (Clague and Jarrard, 1973; Jackson, 1976; This occurred perhaps as early as anomaly 24 but no later than the Jarrard and Clague, 1977; Epp. 1978; McDougall and Duncan, time of anomaly 21, which is approximately the time of the major 1980; Turner and others, 1980; and Duncan and Clague, 1985) change in spreading direction between Greenland and Europe {Vogt I. THE HAWAIIAN-EMPEROR VOLCANiC CHAIN PART I 35 and Avery, 1974) and shortly before an apparent increase in the to explain how a linear chain of volcanoes might be progressively frequency of geomagnetic reversals (jacobs, 1984) The change in erupted onto the sea floor, but most are highly generalized and suffer anomaly orientation can also be correlated with numerous events from lack of detail. Few of the hypotheses address all of the associated with worldwide reorganization of plate motions (Rona kinematic and petrological issues, and none seems to be amenable to and Richardson, 1978~ experimental test. Nonetheless, they are interesting speculations on The early magnetic time scales of Heirtzler and others (1968) solutions to an extremely difficult problem. and LaBreque and others (1977) put anomaly 21 at about 54-53 All of the proposed mechanisms can be grouped into four basic Ma and 52-51 Ma (corrected for new K decay and abundance types: constants), respectively, which implies a lag of at least 10 m.y. 1. Propagating fracture driven by lithospheric stresses. between the reorganization of Pacific magnetic anomalies and the 2. Thermally or chemically driven convection. formation of the Hawaiian-Emperor bend at 43.1 ± 1.4 Ma 3. Melting caused by shear between the lithosphere and the (Dalrymple and Clague, 1976). More recent time scales, however, asthenosphere. have narrowed this somewhat awkward gap. Ness and others 4. Mechanical injection of heat into the lithosphere. (1980) put anomaly 21 at about 49-48 Ma, Lowrie and Alvarez (1981) at about 48.5-47.5 Ma, and Butler and Coney (1981) at about 47-46 Ma. As suggested by Butler and Coney, a lag of 3-4 PROPAGATING·FRACTURE HYPOTHESES m.y. is close enough to suggest a causal relationship between the relative motion change represented by the magnetic bight and the Dana (1849) was the first to associate the Hawaiian volcanic absolute change represented by the Hawaiian-Emperor bend. chain with crustal fracturing. He proposed that the Hawaiian and Gordon and others (1978) suggested that the change in other volcanic chains in the Pacific were each emplaced along a series direction of the Pacific plate at -43 Ma was caused by the of short echelon fractures (or "rents") that were widest at the development of new trenches along the southwestern boundary of the southeast end where volcanism was the most prolonged. He consid plate. These new trenches, which replaced an earlier set of ridges ered these fractures to be part of a worldwide system reflecting and transform faults, were the result of rifting of Australia from tension in the crust resulting from cooling of the Earth from an Antarctica and the accompanying convergence of the Australia initially molten state. S. Powers (1917) agreed that the eruptions Indian and Pacific plates. Gordon and others (1978) suggest that occurred through a superficial set of echelon fractures following the some time would have elapsed before the subducting plate would trend of the chain, but he attributed the trend to some deeper seated have been long enough and dense enough to exert sufficient torque on lines of weakness. Chubb (1934) thought that the Hawaiian swell the Pacific plate to change its direction of motion. This could explain represented the surface manifestation of a broad anticline trending in the lag between the timing of reorientation of the magnetic anoma the direction of the chain and produced by compression oriented lies, which record the change in relative plate motion, and the age of north-northeast and south-southwest. He proposed that the the Hawaiian-Emperor bend, which records the change in absolute Hawaiian volcanoes erupted along strike faults and dip faults atop plate motion. The duration of the lag time would depend on the rate and aligned with the anticline. of plate convergence. As noted by Gordon and others (1978) a lag Beta and Hess (1942) found no evidence of vertical displace time of perhaps as much as 10 m. y. might be explained if con ment along fault scarps but thought that the chain might be the vergence were sufficiently slow. Their mechanism is more plausible, manifestation of a great transcurrent strike-slip fault resulting from however, if the lag can be shortened to a few million years, as now crustal shortening within the Pacific basin caused by Tertiary seems likely. volcanism along the margins of the basin. In view of the Earth's sphericity, the straightness of the chain indicated to them that the fault plane was essentially vertical. Considering the strength and HAWAIIAN HOT·SPOT MODELS thickness of the ocean crust, they thought that an anticline the Although there is now little doubt that the Hawaiian-Emperor dimensions of the Hawaiian swell was unlikely and proposed instead Chain owes its origin to a hot spot that has been approximately fixed that the swell represented a thick lava pile related to the presumed with respect to the Earth's spin axis throughout the Cenozoic, there fault zone. Dietz and Menard (1953) thought this idea improbable is scant information concerning the exact mechanism involved. Even because of the enormous volume of lava that would be required to the term "hot spot" may be misleading, for excess heat is not produce the swell. necessarily involved. Alternatively, it could be the result of pressure Other early authors subscribed to the idea that the Hawaiian release in a mantle source area (Green, 1971; McDougall, 1971; Chain developed atop a propagating fracture (for example, Stearns, Jackson and others, 1972). 1946; Eaton and Murata, 1960; Jackson and Wright, 1970), but A successful hypothesis for the Hawaiian hot-spot mechanism they were vague or noncommital as to the cause of the rupture. must explain the propagation of volcanism along the chain, the near Most recent authors who have advanced propagating-fracture fixity of the hot spot, the chemistry and timing of the eruptions from hypotheses have attempted to relate the cause of the fracture to either individual volcanoes, and the detailed geometry of volcanism, local or regional stress fields within the Pacific plate. Green (1971) including volcano spacing and departures from absolute linearity. suggested that divergent flow vectors caused by the movement of the Over the past decade or so several mechanisms have been advanced plate over an imperfect sphere, that is, an uneven upper mantle 36 VOLCANISM IN HAWAII surface, caused local tension and intermittent failure of the A SEA lEVEL lithosphere. The fracturing would allow rapid upwelling and partial Oceanic crust melting of material from the low-velocity zone. One problem with r M-discontinuity this hypothesis is the means by which the irregularities on the Lithosphere asthenosphere are maintained, but Menard (1973) suggested that ----/- such persistent asthenospheric "bumps" might be caused by a rising Low thermal plume in the mantle. Asthenospheret velocity McDougall (1971), following the ideas of Green (1971), lone proposed that the physical feature that subjected the plate to local j tension might be either a thermal high or an incipient upwelling B caused by a local concentration of heat-producing radioisotopes. ~~T~:'~ According to McDougall's model, fracturing results in the diapiric /,',',':-:' rise of peridotitic material from the asthenosphere into the lithosphere ==- I -:\ (fig. 1.13A, B), where partial melting then generates tholeiitic ~ magma. Movement of the plate and counterflow of the asthenosphere ---0% -',,------eventually decapitate the diapir, but replacement of material from - -:%0' deeper levels of the asthenosphere perpetuates the high and a new '? diapir is created (fig. 1.13C, D). Noting that the rate of propaga c tion of volcanism along the Hawaiian Chain is slightly more than twice the half-spreading rate of the East Pacific Rise, McDougall concluded that there must be counterflow of material in the asthenosphere in a zone of thickness comparable to that of the lithosphere. Jackson and others (1980) showed thai it was not possible to reconcile equal-but-opposite hot-spot motion with the paleolatitude of Suiko Seamount if the counterflow had persisted throughout the history of the Hawaiian-Emperor Chain. Hot-spot countermovement until the time of the bend followed by latitudinal stability from then to the present is, however, kinematically per missible. Another mechanism for producing a local stress field and lithospheric ruplure was proposed by Walcoll (1976), who related the stress to the volcanic load on the lithosphere. He suggested that large volcanoes will produce lithospheric stresses during growth that may be large enough to cause disruption of the plate. If the plate is under a normal state of horizontal compression, then the failure of o 50 100 KILOMETERS NO VERTICAL the lithosphere will occur preferentially parallel to the direction of the I EXAGGERATION compressive stress. The direction of rupture will remain linear as FIGURE I. 13.-Schcmalic diagram of McDougall's (1971) propagating-fracture long as the ambient stress direction remains constant, and the rate of hypothesis. Propagating tensional fracture allows diapiric upwelling from propagation will depend on the speed of formation of the load. asthenosphere (A) and partial melting (B~ Relative motion between lithosphere and asthenosphere (arrow along left margin) eventually decapitates diapir (C) and Noting the rapidity with which Hawaiian volcanoes form, Walcott cycle begins at a new position (D~ The shaded zone represents peridotitic material concluded that the propagation of volcanism along the Hawaiian thai is the source rock of lhe lava. From McDougall. chain must be limited by the availability of magma source material. Thus, the mechanism would be self-perpetuating and self-regulating. Although this mechanism will result in a line of volcanoes, it does not explain the observed age progression nor does it account for hot-spot fixity, but it might be locally important and explain the detailed extensional strain resulting from tension within the Pacific plate, but distribution of volcanoes within the Hawaiian Chain (Walcott, they did not speculate on the ultimate cause of the stresses. Jackson 1976). and Shaw (1975) developed this idea more fully and extended it to Expanding on the original idea of Dana (1849), Jackson and other chains in the Pacific. They argued that linear hot-spot chains others (1972) observed that the individual volcanic centers of the track and record the states of stress in the Pacific plate as a function Hawaiian-Emperor Chain appear to lie on short, sigmoidal, over of time, and that the stress was reflected in the detailed geometry of lapping loci that are echelon in a clockwise sense in the Hawaiian volcanoes within a chain, that is, in the orientation of the volcanic Chain and in a counterclockwise sense in the Emperor Chain (fig. loci, which represent the injection of magma along lines perpen 1.14), although the laller was based on inadequate bathymetric dicular to least principal stress directions. On the basis of their data. They proposed that the pattern of loci may be caused by analysis of the Hawaiian-Emperor, Pratt-Welker, Tuamotu, and I. THE HAWAIIAN-EMPEROR VOLCANIC CHAIN PART I 37 f----24· o 200 KILOMETERS '---__-'-__----l' ----!------18· 1560 EXPLANAnON x Topographic high • Bouguer gravity anomaly high t> 250 mGall Loci of shield volcanoes ~ Area of closed low HAWAIIAN·EMPEROR BEND I 30° ---+------ I i 1700 French Frigate Shoals 170 0 o 1000 KILOMETERS , _____..1- _ ___J FIGURE 1.14. - Loci of shield volcanoes in Hawaiian-Emperor Chain according to Jackson and others (1972). Inset shows detailed relation between topographic highs, Bouguer gravity anomaly highs, and loci for principal Hawaiian Islands. Contour interval is I km; hachures indicate area of closed low. 38 VOLCANISM IN HAWAII Austral-Ellice-Gilbert-Marshall Chains, they concluded that the A stress orientations since the time of formation of the Hawaiian Emperor bend were caused by a right-lateral rotational couple acting within the plane of the Pacific plate. This couple resulted in the minimum principal stress oriented in a northeast-southwest Brittle direction. Before the time of the bend, the rotational couple was left fracture lateral and the minimum stress was oriented north-northwest and south-southeast. The curvature in the volcanic loci, they proposed. reflects episodic swings of the minimum-stress directions that aver aged about 12 m.y. per episode and were perhaps a consequence of episodic changes in the force vectors at plate boundaries. Jackson and Shaw (1975) were uncertain about the exact causes of the stress field within the Pacific plate, but noted that possible contributors included convergence and divergence at plate boundaries, varying convection rates in the asthenosphere, and volume changes within the plate resulting from changing pressure and temperature. On the basis of an analysis of volcano spacing and the relation of volcanic chains to preexisting plate structures, Vogt (1974) suggested that the factors that controlled the path of hot-spot chains are not clearly of one origin, but included simple shear, reactivated sea-floor-spreading structures, and local stresses. He concluded that the sigmoidal loci (fractures) postulated by Jackson and others (1972) for the Hawaiian Chain had no counterpart in other chains, although Jackson and Shaw (1975) claimed 10 have found a similar pattern on other chains in the Pacific. B Solomon and Sleep (1974) preferred the propagating-fracture hypothesis, in part because it avoided the necessity of an abnormal and unknown source of heat in the asthenosphere. They emphasized that the stresses in the Pacific plate can be explained entirely in terms Tensional of the forces acting on plate boundaries, and that such mechanisms "fracture have the attractive feature of being amenable to numerical treatment. They proposed that the continued motion of the plate with respect to the boundary force field and to secondary convection cells in the asthenosphere might cause a linear propagating fracture as new parts of the plate moved into zones of tension, and that such a tensional fracture would permit the passive upwelling of volcanic material from below. This model offers no explanation why Hawaii is located where it is. In addition, passive mantle upwelling seems inadequate to produce the enormous volume of lava that comprises the Hawaiian Islands. Compression / Turcotte and Oxburgh (1973, 1976, 1978) also subscribed to c / propagating tensional fractures as a possible cause of linear midplate -- volcanism. They noted that although brittle failure may occur at the surface of a plate, plastic failure is more likely at depth where lithostatic pressure is large compared with the yield stress. The oretically, plastic and brittle failure will occur at angles of 35° and 45', respectively, 10 the direction of lension (fig. I. I SA). Possible causes of tension include thermal stresses in the cooling and thicken ing plate as it moves outward from the spreading ridge and fracture membrane stresses caused by the movement of plates on the surface of the nonspherical Earth (fig. 1.158, C). Turcotte and Oxburgh FIGURE 1.1S.-Tensional stresses as a possible cause of propagating fractures in lithospheric plates. A. Orientation of plastic and brittle failure in thin plate under note that the angle between the Hawaiian Chain and the direction of tension (n according to Turcone and Oxburgh (1973, 1976, 1978~ H, Fracture sea-floor spreading, as deduced from magnetic anomalies and in hthospheric plate from tensional stress caused by cooling and thickening of plate fracture zones, is 34°, in good agreement with the predicted value. away from spreading ridge. C, Fracture caused by membrane stresses in They also note that the angle between the trend of the chain and the northward-moving plate on oblate Earth. I. THE HAWAIIAN-EMPEROR VOLCANIC CHAIN PART I 39 loci of Jackson and others (1972) is approximately correct for brittle fracture. The Cook-Austral, Tuamoto-Pitcairn, and Kodiak Spreading ocean ridge Bowie Chains also lie at angles of between 31 0 and 42° to spreading directions, but the angle made the Marquesas is 60°, which is by Volcanic much larger than that predicted by Turcotte and Oxburgh (1978). chain Both plastic and brittle failure, as proposed by Turcotte and Oxburgh, provide a means of propagating a fracture as a function of plate motion and might account for some degree of hot-spot fixity. The thermal mechanism relies on cooling and thickening of the plate as a function of time and distance from the spreading ridge. Once started, the fracture will propagate from a point that remains at a fixed crustal age from the ridge. As these authors point out, fractures due to membrane stresses would be most likely in middle latitudes because the change in the radius of curvature of the Earth is a maximum at a latitude of about 45°. For a plate in the northern hemisphere moving northward, the fracture would propagate south ward from a point that remains latitudinally fixed. This mechanism FIGURE 1.16.-Wilson's proposed possible origin of Hawaiian Chain. If lava is does not, however, account for the great variety of latitudes of active generated in stable core of mantle convection cell and surface is carried along by plate motion, then one source can give rise to a chain of successively extinct Pacific hot spots, the parallelism of Pacific volcanic chains, or the volcanoes. Modified from Wilson (1963), by permission of the National Research Hawaiian-Emperor bend (Solomon and Sleep, 1974). Council of Canada. Handschumacber (1973) advanced three fracture-related explanations for the Emperor Seamount Chain, but he did not extend them to include the Hawaiian Chain. Two of the mechanisms, extrusion along a strike-slip fault and interaction between a stable part of the Pacific plate on the west and a spreading ridge on the east, have since been disproved by the age progression (younger but did not speculate on the ultimate cause of the lava source, southward) of the Emperor volcanoes. The third mechanism, sec The hypothesis that has undoubtedly received the most atten ondary activity along a zone of weakness between eastern and tion since Wilson's is that of Morgan (1971, 1972a, b) wbo western parts of the plate, invokes preexisting structural control, proposed that the Hawaiian and other Pacific hot spots were narrow but, like all propagating fracture hypotheses, does not provide any thermal zones of upwelling, which he termed "plumes," that originate insight into the lava-producing mechanism. deep within the Earth's mantle, possibly near the core. They arise because of thermal instabilities (excess heat), which cause upward convection of hot plumes of mantle rock in much the same way that THERMAL AND CHEMICAL CONVECTION HYPOTHESES thermal instabilities in the atmosphere cause thunderhead clouds. Numerous authors have associated the Hawaiian Chain with According to this hypothesis, the plumes are of relatively low thermally driven convection in the asthenosphere. Among the ear viscosity, about I 50 km in diameter, and convect upward at a rate of liest were Dietz and Menard (1953) and Menard (1955\ who about 2 m/yr. In addition to providing lava for volcanic chains, hypothesized that the Hawaiian Arch or swell occurred over the plumes are considered by Morgan to be a driving force of plate intersection of two upwelling and diverging convection cells. This tectonics, to be capable of rifting continents, and to occur on would put the lithosphere under tension and produce fracturing as midocean ridges as well as in the middle of plates. Morgan identified the volcanic load increased, providing a reasonable explanation for about 20 hot spots, but subsequent authors have tended to be more the geometry and form of the Hawaiian Arch, Ridge, and Deep. It generous (for example, Burke and Wilson, 1976; Crough, 1983). does not, however, account for the constant rate of propagation of One aspect of Morgan's hypothesis that has proven extremely volcanism along the chain, although in 1955 this was poorly known. important to the study of plate tectonics, whether or not hot spots are Although he did not discuss the Hawaiian Chain, Wilson (1962) actually plumes, is the concept that hot spots are fixed relative to one showed it to be coincident with an early Tertiary ridge which he another and to the Earth's spin axis. As we discussed earlier, hot suggested formed by diverging convection cells. spot fixity appears to be generally true for long periods of geologic Wilson (1963a, b, c, d) was the first to suggest a thermal time. and thus hot spots provide a stable reference frame for studies convection mechanism that specifically addressed the age progression of absolute plate motions, in the Hawaiian and eight other parallel chains in the Pacific. He Morgan (1972a, 1972b) observed that most hot spots were speculated that the source of lava resided in the stagnant, or at least characterized by a positive gravity anomaly and a topographic high. more slowly moving, region of a mantle convection cell (fig. I. 16 ~ both of which, he said, are symptomatic of rising thermal currents in Spreading of the sea floor above this fixed source would result in an the mantle. Morgan calculated that as few as 20 plumes could bring age-progressive chain of volcanoes. Wilson (I 963a) tentatively put up from depth an estimated 500 km3/yr of mantle material and half the source at a depth of about 200 km, below the low-velocity zone, of the total heat flow from the Earth. 40 VOLCANISM IN HAWAII \Vilson (1973) endorsed the plume hypothesis and likened cooling nebula. Thus, the primitive deep mantle was a male plumes to other natural diapiric mechanisms such as salt domes, enriched in Ca, AI, 11, and the refractory trace elements, indue thunderheads, and volcanic pipes. Menard (1973) noted that the U and Th. This material, being less dense than the overlying [ay. Hawaiian, Austral-Cook (Macdonald Seamount), and Gulf of rose as chemical plumes through buoyancy early in Earth's hist Alaska hot spots all lie on the updr.ft side of asthenospheric bumps and partially melted to yield anorthosites. Present-day hot S1 and concluded that equally persistent rising plumes were required to occur above the mantle residua of this partial melting. These plu sustain the asthenospheric relief at sites not associated with hot spots. provide heat to the base of the lithosphere because they are enric Strong (1974) noted that the compositions of Kilauea and Mauna in heat-producing elements, principally U and Th, and so consti Loa lava were not the same, concluded that the Hawaiian plume what could be called radioactive hot spots. Chemical plumes m was probably not the direct source of lava, and questioned whether explain both asthenosphenc bumps and also the episodic natur. Morgan's plumes were necessarily zones of mass transport. Alter volcanism. Anderson proposed that the rapid withdrawal of hea' natively, he suggested they might be zones of high thermal con magma could periodically outstrip heat production and there ductivity or concentrated diffusion. temporarily halt magma generation. However, one would think Morgan (1972b) proposed four tests of the plume hypothesis, the chemical inhomogeneities should be seismically detectable. including seismic detection, prediction of plate motions from plume Richter (1973) and Richter and Parsons (1975) have, dynamics, evaluation of the necessity of plumes for heat transport gested that the Hawaiian-Emperor Chain and other linear ch from the deep mantle, and correlation of changes in Cenozoic and might be a consequence of the nonlinear interaction of two diffe Cretaceous spreading patterns with the disappearance or emergence scales of mantle convection, one involving sea-floor spreading of new hot spots. Of the four, only the seismic test had any real the return flow necessary to conserve mass, and the othe potential for yielding a conclusive answer. Davies and Sheppard Rayleigh-Benard convection reaching to depths of about 650 (1972), Kanasewich and others (1972, 1973), and Kanasewich This latter convection forms rolls whose axes initially are ali~ and Gutowski (1975) analyzed seismic rays passing beneath the perpendicular to the spreading direction. In time, however, Hawaiian Islands from earthquakes in the southwest Pacific. They latitudinal rolls give way to longitudinal rolls with axes parallel tc concluded that there is a zone of abnormally high velocities near the direction of plate motion (fig. I. 17). The time for the transitio core-mantle boundary beneath Hawaii and that the seismic data are occur depends on the spreading velocity, but may be as slier generally consistent with Morgan's plume hypothesis, although there about 20 m.y. for a fast (about 10 cmlyr) plate like the Pacific p were no data indicating an extension of the velocity anomaly upward Longitudinal rolls will generate alternating bands of tension through the upper mantle. The interpretation of the seismic data was compression in the overlying plate. Linear volcanic chains rr questioned by Wright (1975) and Green (1975), who concluded form along the zones of tension and, either because of moclulatic that the observed travel time anomalies were most likely the result of convection amplitude along the roll or because of the [rae upper mantle inhomogeneities beneath the seismic detector arrays in properties of the plate, could propagate opposite to the directic western North America. From a study of teleseismic arrivals from spreading. A feature of this mechanism is that ages out of order 55 earthquakes recorded at 21 stations on Hawaii, however, occur. In addition, an age gap of some tens of millions of years c Ellsworth and others (1975) found evidence of lower than average occur near the bend in the Hawaiian-Emperor Chain because 0 velocities at depths of 30-50 km beneath the island. Whether this time required for a new set of longitudinal rolls to be establi anomaly extends into the asthenosphere is unknown. Thus, the seismic evidence for a thermal plume beneath Hawaii appears to be, at best, inconclusive. One difficulty with the plume hypothesis is that narrowly confined convection is unstable in fluids with high Prandtl numbers (kinematic viscosity divided by thermal diffusivity) such as mantle Spreading rridge material (Turcotte and Oxburgh, 1978). Narrow plumes might be sustained, however, if confined to the upper mantle and heated from below by a lower mantle source (Turcotte and Oxburgh, 1978). Another problem is that the amount of partial melting that would result from the adiabatic decompression of mantle material rising from the core-mantle boundary is much too high to result in Hawaiian basalt (Turcotte and Oxburgh, 1978) This objection might not apply if mantle plumes are a source of heat for melting of the lower lithosphere or the uppermost asthenosphere rather than a direct source of magma. An alternative to thermal plumes, proposed by Anderson FIGURE 1.17.-Schematic diagram of large-scale asthenospheric Aow rela (1975), is that the plumes are relict compositional conduits. Accord sea-floor spreading and superimposed small-scale longitudinal rolls. Volcanic ing to Anderson's hypothesis, the Earth accreted inhomogeneously might occur in zone of tension between diverging rolls and would prot and in the sequence in which compounds would condense from a opposite 10 direction of spreading. From Richter and Parsons (1975~ 1. THE HAWAIIAN-EMPEROR VOLCANiC CHAIN PART I 41 following a change in spreading direction. The age data for the 0 r--=--,------,-----,-----,------, Hawaiian-Emperor Chain (fig. I.S), however, show that the propa- gation is continuous around the bend, although seamounts are sparse on the westernmost Hawaiian Ridge. Another feature of the longitu e: 0.011 Kauai -c dinal roll model is that parallel volcanic chains should be spaced at w >- some multiple of twice the depth of the convecting layer, which is in 0.017 Waianae w c,'" accord with the geometry of the major Pacific chains for a convecting 0.023 Kooteu '" depth of about 600 km (Richter, 1973). w'" 10 >-w 0.031 0.035 i="z SHEAR-MELTING HYPOTHESES w U Shear melting with thermal feedback to regulate the propaga ;!: z· tion rate was proposed by Shaw (1973) to explain the nonlinear 0 i= time-distance-volume relations along the Hawaiian Chain noted by -c o Jackson and others (1972) and Swanson (1972) (fig. I. 18). -c c, According to his hypothesis, the hot spot is the result of a delicately 0 20 '"c, balanced thermomechanical process that derives energy from plate u Z motion and is regulated by a feedback process inherent in the -c u physical properties of the rocks involved. In principle, the idea is ~ 0 quite simple and is based on the observation that a viscous medium > u, will rise in temperature when sheared. Shear occurs within a finite 0 >- • Kilauea zone between the lower lithosphere and the upper asthenosphere t: u 0 because of their relative motion. As shear proceeds the temperature ~ w 30 rises and the viscosity decreases within the shear zone. This allows > an increase in the rate of shearing, which in turn produces a further increase in temperature. The increasing temperature eventually results in partial melting and the formation of magma, which rises to the surface to form the volcanoes. The magma carries off excess o 200 400 heat, the temperature decreases rapidly, viscosity increases, and CHANGE IN VOLUME WITH DISTANCE, IN CUBIC KILOMETERS PER KILOMETER meltingstops temporarily as a new cycle is initiated. Each cycle lasts a few million years and is characterized by accelerating propagation FIGURE 1.18. -Change in volume of lava with respect to unit distance versus of volcanism and eruption volume followed by a sudden halt. change in distance with respect to time (velocity of volcanic propagation) for A means of localizing shear melting and fixing the resulting hot principal Hawaiian Islands. Diameter of circles approximately proportional 10 spot relative to the mantle was advanced by Shaw and Jackson apparent eruption rates, which are also given (in cubic kilometersper year) next to circles. From Shaw (1973~ (1973). They proposed that once partial melting began the residua sinks, forming a type of gravitational anchor that reaches down into the mantle, perhaps to the core-mantle boundary (fig. I. 19). The downwelling anchor not only forms a geographic pinning point for the hot spot but also results in the inflow of fresh mantle material beneath the hot spot, which thus is nol limited by supply, There is Dietz and Menard, 1953; Menard, 1955). Only recently, however, strong evidence, however, that the depleted residua from partial has it become clear that the swell may be the result of thermal melting of the most likely parent rocks are less dense than the parent resetting and thinning of the aging and thickening lithosphere. material and would not sink (see, for example, O'Hara, 1975; Detrick and Crough (1978) observed that long-term rates of Bnyd and McCallister, 1976; Jordan, 1979). Thus, unless the subsidence of volcanoes in the Pacific are higher than can be source of Hawaiian basalt is something quite unusual, the formation accounted for by the subsidence that accompanies the cooling and of a gravitational anchor seems unlikely, and the shear-melting thickening of the lithosphere as it moves away from the spreading hypothesis suffers from the lack of both a starting mechanism and a ridge (parsons and Sclater, 1977: Schroeder, 1984~ They pro means of localization. posed that the excess subsidence is the result of thermal resetting of the lithosphere as the aging plate rides over the hot spot. The resetting is accompanied by lithospheric thinning and a rise in the HEAT·INJECTION HYPOTHESIS elevation of the sea floor, The rapid subsequent subsidence then It has long been known that the Hawaiian hot spot, among represents a gradual return of these shallow areas to normal depths, others, is associated with a broad topographic anomaly on the ocean that is, depths commensurate with the age of the sea iloor (see also floor, the Hawaiian swell, which has been attributed to some sort of Crough, 1979, 1983: Epp, 1984t The hypothesis of thermal thermal anomaly for more than three decades (see, for example, resetting is supported by anomalously high heat Row along the 42 VOLCANISM IN HAWAII A Detrick and Crough (1978) recognized that the major problem with their thermal model for the Hawaiian swell is that it requires extremely rapid heating of the lithosphere; a heat flux more than 40 times normal is indicated, if the heating is entirely by conduction. This is because the kinematics of plate motion relative to the hot spot requires the swell to rise in only a few million years, whereas it would take about 100 m.y. at twice the normal heat Aux to raise the swell. This problem, however, may not be as serious as it once seemed. More recent modeling by Nakiboglu and Lambeck (1985) demon ~ : strates the sensitivity of these calculations to the lower boundary ------condition. They argue that most of the Hawaiian swell can be produced by thermal conduction, but a small dynamic component may also be required to support the swell. Another potential solution to this problem, proposed by McNutt (1984), is lithospheric delamination, a process invoked by Bird (1979) to explain vol canism in continental interiors. According to this hypothesis, a strip of the lower lithosphere separates from the upper lithosphere and descends into the asthenosphere. This produces the sudden rise in temperature at the base of the remaining lithosphere required to B Northwest Southeast produce the swell without invoking an unreasonable heat Aux. The lateral resistance of the descending strip might also provide the necessary stability of the hot spot with respect to the mantle. It is 6:1~_lithosphere unclear how delamination might begin, but once started theory •, suggests that it can propagate at plate velocities (Bird and , , Baumgardner, 1981). '- \ Asthenosphere , One problem with delamination is that it requires the sinking into the asthenosphere of the lower lithosphere, which is thought to be one component of the source of ocean-island basalt. For Hawaii the proposed depth of delamination, that is, the thickness of the lithosphere over the hot spot, is slightly less than 30 km (McNutt, 1984), a depth considered to be well above the source region of Hawaiian basalt. It is also clear from pressure-temperature relations that the descending slab would not melt (and if it did the residua would rise rather than sink). Therefore, Hawaiian basalt would have to be generated from the material of the upper asthenosphere, although at lower lithosphere depths, and the lithosphere asthenosphere boundary would be a purely mechanical one (that is, with no compositional differences across the boundary). In summary, geophysical models for the Hawaiian hot spot tend to be highly generaliz.ed and difficult if not impossible to test. None has yet been advanced that satisfactorily explains all of the Mantle Core geometric, kinematic, physical, and chemical observations from the Hawaiian-Emperor Chain. Although many intriguing and clever FIGURE 1.19. -Schematic views of possible downwelling of dense residua from tholeiitic melting. A, Plan view showing hypothetical flow lines in asthenosphere ideas have been advanced, the hot-spot mechanism is still somewhat along horizontal plane taken at lime near culmination of melting episode. B, mysterious. Detrick and Crough's (1978) idea that the Hawaiian Vertical section showing proposed gravitational anchor. From Shaw and Jackson swell is caused by thermal resetting of the aging ocean crust implies ( 1973~ that hot spots are indeed hot. In addition, the possibility that the swell is dynamically supported (Detrick and Crough, 1978) implies that material wells up beneath the lithosphere. Petrologic studies indicate that Hawaiian lava is generated from mantle sources Hawaiian Ridge (Detrick and others, 1981). The concept of consisting of at least 3 geochemical components; one of these is a lithospheric thinning over hot spots is substantiated by the flexural primitive undegassed component. The cause of the Hawaiian hot data, which indicate that the lithosphere over hot spots is much spot is still unknown, but present hypotheses are consistent with thinner than that of comparable age flexed at subduction zones Morgan's plume hypothesis in which hot primitive mantle material (McNutt, 1984). ascends beneath the ocean lithosphere below Hawaii and reacts with 1. THE HAWAIIAN-EMPEROR VOLCANIC CHAIN PART 1 43 the lithosphere to produce the compositional range of Hawaiian 1301-2-3. lava. Chen, c.-y, and Frey, F.A, 1983, Origin of Hawaiian tholeiites and alkalic basalt: Nature, v. 302, p. 785-789. ---1985, Trace element and isotope geochemistry of lavas from Haleakala Volcano, East Maui: Implications for the origin of Hawaiian basalts: Journal REFERENCES Geophysical Research, v. 90, p. 8743-8768. 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The Leeward Islands: American journal of Science, Series 5, v. 12, p. p. 336-352. ---1947, Geology and ground-water resources of the Island of Molokai, ---1928, Petrology of the Hawaiian Islands: VI Maui: American Journal of Hawaii (geologicmap of Molokai enclosed): Hawaii Division of Hydrography, Science, Series 5, v. 15, p. 199-220. Bulletin II, 113 p. Watts. A.B., 1978, An analysis of isostacy in the world's oceans l. Hawaiian Stearns, H.T., and Vaksvik, K.N., 1935, Geology and ground-water resources of Emperor Seamount Chain: journal of Geophysical Research, v. 83, p. the Island of Oahu, Hawaii: Hawaii Division of Hydrography, Bulletin I, 479 5989-6004. p- Wentworth. C.K., 1925, The geology of Lanai: Bernice Pauhi Bishop Museum, Steiger, R H., and Jager, E.. 1977, Subcommission on geochronology: Convention Bulletin 24, 72 pp. on the use of decay constants in gee and cosmochronlcgy: Earth and Planetary ---1927, Estimates of marine and fluvial erosion in Hawaii: journal of Geology Science Letters, v. 36, p. 359-362. v. 35, p. 117-133. Stille, P., Unruh, D.M., and Tatsumoto, M., 1983, Pb, Sr, Nd, and Hf isotopic West, H.B., and Garcia, M.o., 1982, Composition and evolution of the alkalic evidence of multiple sources for Oahu, Hawaii basalts: Nature, v. 304, p. cap stage lavas from Mauna Kea Volcano, Hawaii: Ecs, Transactions, 25-29. American Geophysical Union, v. 63, p. 1138. Strong. D. F., 1974, Volcaniccouples and deep mantle plumes: Nature, v. 247, p. White, R. W., 1966, Ultramafic inclusions in basaltic rocks from Hawaii: Miner 191-193. alogie und Petrographic Mitt., v. 12, p. 245-314. Swanson, D.A, 1972, Magma supply note at Kilauea Volcano, 1952-1971: White, W.M., and Hofmann, AW., 1982, s- and Nd isotope geochemistry of Science, v. 175, p. 169-170. oceanic basalts and mantle evolution: Nature, v. 296, p. 821-825. Takayama, T., 1980, Calcareous nannofossil biostratigraphy, Leg 55 of the Deep Wilkes, c., 1845, Narrative of the United States Exploring Expedition, Sea Drilling Project, in Jackson, E. D., Koisumi, l., and others, Initial 1838-1842,4: Philadelphia, 539 p. Reports of the Deep Sea Drilling Project, v. 55: Washington, U.S. Govern Wilson, j. T, 1962, Cabot Fault, an Appalachian equivalent of the San Andreas ment Printing Office, p. 349-364. and Great Glen faults and some implications for continental displacement: Tatsumoto, M., 1966, Isotopic composition of lead in volcanic rocks from Hawaii, Nature v. 195, p. 135-138. lwo jima. and japan: journal Geophysical Research, v, 71, p. 1721-1733. ---1963a, A possible origin of the Hawaiian Islands: Canadian journal of ---1978, Isotopic composition of lead in oceanic basalt and its implication to Physics, v. 41, p. 863-870. mantle evolution: Earth and Planetary Science Letters, v. 38, p. 63-87. ---1963b, Continental drift: Scientific American, v. 208, no. 4, p. 86-100. Tayama, R, 1952, On the near-Japan bathymetric chart (introduction to the ---1963c, Evidence from islands on the spreading of ocean Roors: Nature, v. I. THE HAWAIIAN-EMPEROR VOLCANIC CHAIN PART 1 49 197. p. 536-538. in the water column above Loihi (Hcribe and others, 1983; Kim and Craig, 1983) ---1963d, Hypothesis of Earth's behavior: Nature, v. 198. p. 925-929. and the presence of water-temperature anomalies recorded by the ANGUS camera ---1973, Mantle plumes and plate motions: Tectonophysics, v. 19. p. sled (Malahoff and others, 1982~ 149-164. \Vise, W.S., 1982, A volume-time framework for the evolution of Mauna Kea Kilauea Volcano (IJ-The lava of Kilauea, currently active and historically Volcano, Hawaii; £os, Transactions, American Geophysical Union, v. 63, p. the most active volcano in Hawaii, can be divided into the older Hilina Basalt and 1137. the younger Puna Basalt, which are separated by the Pahala Ash. The exposed lava Worsley, JR.. 1973, Calcareous nannofossils: Leg 19 of the Deep Sea Drilling consists of tholeiitic basalt and picritic tholeiitic basalt that issued from the 3-km by 5 Project, in Creager. 1.5., Scholl, D.W., and others, Initial Reports of the km summit caldera and the two rift zones. The rift zones extend to the east and the Deep Sea Drilling Project, v. 19: Washington, U.S. Government Printing southwest, with the east rift zone extending nearly 50 km from the summit caldera to Offi". p. 741-750. Cape Kumikahi at the northeast corner of the island and for at least an additional 90 Wright, C, 1975, Comments on 'Seismic array evidence of a core boundary source km beneath the sea. for the Hawaiian linear volcanic chain' by E. R. Kenasewicb and others: Journal of Geophysical Research v. 80, p. 1915-1919. Mauna Loa Volcano (2).-1be lava of Mauna Loa is divided into the Ninole Wright, TL.. 1971. Chemistry of Kilauea and Mauna Loa lava in space and time: Basalt (oldest), the Kahuku Basalt, and the Kau Basalt [youngest], The Kahuku U.S. Geological Survey Professional Paper 735, 40 p. and Kau are separated by the Pahala Ash and are thought to be coeval with the ---1973, Magma mixing as illustrated by the 1959 eruption, Kilauea Volcano, Hilina Basalt and Puna Basalt, respectively, of Kilauea. The exposed lava is all Hawaii: Geological Society of America Bulletin, v. 84, p. 849-858. tholeiitic basalt and picnuc tholeiitic basalt that issued from the 2.5-km by 4-km ---1984, Origin of Hawaiian tholeiite: A metasomatic model: Journal of summit caldera, named Mokuaweoweo, and two rift zones. The rift zones extend Geophysical Research. v. 89, p. 3233-3252. southwest and east-northeast. The southeastern and the southwestern slopes of Wright, TL., and Clague, D.A., in press, Petrology of Hawaiian lava: Geologic Mauna Loa are steepened by downfaulting along the Kaoiki and Kealakekua fault Society of America, Decade of North American Geology, the Eastern Pacific systems. Mauna Loa last erupted in 1984. Possible remnants of two earlier shield Region. volcanoes are exposed in the Ninole Hills (Ninole Basalt) and in the vicinity of Wright, T L., and Fiske, R.S., 1971, Origin of the differentiated and hybrid lavas Kulani. Neither of these earlier shield volcanoes is well delineated and both may be of Kilauea Volcano, Hawaii: Journal of Petrology, v. 12. p. 1-65. merely deeper parts of the Mauna Loa shield uplifted along normal faults in a manner Wright, TL., Shaw, HR.. Tilling, R.I., and Fiske, R.S., 1979, Origin of analogous to that in the Hilina fault system near Puu Kapukapu. With the exception Hawaiian tholeiitic basalt; a quantitative model: Hawaii Symposium on Intra of numerous 14C ages, the sole published age data for Mauna Loa were obtained by plate Volcanism and Submarine Volcanism, Abstracts, p. 104. Evernden and others (1964) on two samples from the Ninole Basalt. One sample York, D., 1969, Least squares fitting of a straight line with correlated errors: Earth contained negligible radiogenic Kaula Island (l5A).-Kaula Island is a small tuff cone on a large submarine probably erupted during the shield stage. Four dated samples have a mean age of edifice. The edifice almost surely represents a separate shield volcano related 10 the 12.0±0.4 Ma. Hawaiian Islands, hut it has not been sampled. The tuff cone is probably a vent of Broo~.s Ban~ (28). - Three samples have been analyzed from dredge 41 of the the alkalic rejuvenated stage. Garcia. Frey and Grooms (in press) described second leg of the Hawaii Institute of Geophysics cruise 72-07-02 (Clague, 1974a; accidentalblocksof tholeiitic basalt. basanite, phonolite, and ultramafic xenoliths thai Garcia. Frey, and Naughton, in press). Two of these samples are hawaiite, probably occur in the tuff. from the same Row, and the third sample is an olivine basalt transitional between Garcia, Grooms, and Naughton (in press) obtained K-Ar ages for two tholeiitic and alkalic basalt. The hawaiite probably erupted during the alkalic phonolite blocks and a basanite from the tuff; they determined ages of 4.00±O.09 postshield stage and the transitional basalt during either the late shield stage or the and 4.22±O.25 Ma for phonolitesamples, 3.98±O.70 Ma for a biotite separated caldera-collapse phase. The hawaiite and alkalic basalt have a mean age of from the phonolite. and 1.8±O.2 Ma for the basanite. 13.0±0.06 Ma. On the basis of the composition and age of the phonolite, we propose that the phonolite is from the alkalic postshield stage, the basanite blocks are from rejuve SI. Rogatien Bank (29).-A singlesample has been analyzed from dredge 44 nated-stage flowsunderlying the tuff cone (Garcia, Frey, and Grooms, in press), and of the second leg of the Hawaii Institute of Geophysics cruise 72-07-02 (Clague, tholeiitic basalt represents the shield stage. 1974a} The sample is an aphyric hawaiite that probably erupted during the alkalic Nihoa Island (l7).-Nihoa Island is a remnant of a large tholeiiticshield with postshield stage; it has not been dated. flows dipping 5°_10° to the southwest. All the flows exposed on Nihoa are of GardnerPinnacles (30). -The two rocks that constitute Gardner Pinnacles an tholeiitic basalt, and they range from aphyric to porphyritic in texture (Dalrymple the westernmost subaerial exposures of volcanic rock in the Hawaiian Chain. The and others, 1974} alkalic basalt Rows that make up the rocks dip 1Soto the west and are cut by severe Funkhouser and others (1968) obtained an age of 7.5±OA Ma for a single east-trending dikes (Dalrymple and others, 1974} Dredged samples of geo sample from Nihoa Island. Dalrymple and others (1974) reported a best weighted chemically similar, though less differentiated, alkalic basalt were recovered in dredge mean age of 7.2±0.3 Ma for six samples of tholeiitic basalt from the island. 37 from the second leg of the Hawaii Institute of Geophysics cruise 72-07-m Ran~ Unnamed Seamount (/9).-A single sample dredged by the Hawaii Institute (Clague, 1974; Garcia, Frey, and Naughton, in press). A later dredge on the of Geophysics from this seamount has been analyzed (Garcia, Frey, and Naughton, of Gardner Pinnacles (HIG dredge 6-7; see Garcia, Frey, and Naughton, in press in press} The samples in dredge 9-11 are moderately altered picritic tholeiitic to recovered largely unaltered picntic tholeiiticbasalt. We infer that the picritic tholeiitir transitional basalt with about 30 percent olivine phenocrysts. These probably basalt erupted during the shield stage and the alkalic basalt Rows during the erupted during the late shield stage or the caldera-filling phase. The seamount is poetshield stage. Additional samples have recently been recovered during Hawai KK84~04-28-0) undated. Institute of Geophysics cruise from a number of dredge stations 01 Gardner Pinnacles, but these have yet to be analyzed (Campbell and others, 1984) Unnamed Seamount (20).-On the second leg of the Hawaii Institute of Samples from the island were too altered for dating (Dalrymple and others Geophysics cruise 72-07-02, dredge SI recovered tholeiitic basalt with 20 percent 1974), but Garcia, Frey, and Naughton (in press) obtained a weighted mean age 0 phenocrysts of augite, plagioclase, and olivine, and aphyrjc alkalic lava of basanite 12.3::: 1.0 Ma for two dredged samples of alkalic basalt and one of tholeiiticbasalt composition (Clague, 1974a; Garcia, Frey, and Naughton, in press} These rocks probably erupted during the shield and the alkalic rejuvenated stages, respectively. LJy.san Island (36).-A single dredge during U.S. Geological Survey cruise Garcia, Frey, and Naughton (in press) obtained a weighted mean age of 9.6±0.8 LEE8-76-NP recovered a variety of hawaiite and mugearite pebbles (Dalrymple Ma for four analyses of two of the dredged alkalic basalt samples. and others, 1981) that probably erupted during the alkalic postshielcl stage Conventional K-Ar and 4OAr_ 39Ar measurementson five of the samples fall withir Unnamed Seamount (21).-On the second leg of the Hawaii Institute of the range 18.8~21.4 Ma, and 4°Ar_39 Ar incremental heating experimentson thre, Geophysics cruise 72-07-02, dredge 49 recovered tholeiitic to transitional basalt samples gave a mean age of 19.9±0.3 Ma. containing 20 percent phenocrysts of olivine and augite (Clague, 1974a} This lava probably erupted during the shield stage. The volcano is undated. Northamp/on Bank (37).-A Hawaii Institute of Geophysics cruise sampler the south side of Northampton Bank and recovered coral-reef debris, picriti. Necker Island (23).-Samples have been collected from Necker Island tholeiitic basalt, and olivine tholeiitic basalt that probably erupted during the shielr (Dalrymple and others, 1974), and others have been dredged from the submarine stage. Dalrymple and others (1981) reported conventional K-Ar and 4OAr_ 39 A flanks of the volcano during Hawaii Institute of Geophysics cruises 72-07-02 (second age data for three dredged samples of tholeiitic basalt. Only one of the samples gave i leg, dredge 48) and KKB4-0B-06-01 (Clague, 1974a; Campbell and others, 4OAr-39Ar age spectrum plateau. The inferred age for that sample is 26.6±2.: 1984} The subaerial samples are mostly picritic tholeiitic basalt collected from Rows Ma. dipping SO_10° to the north-northwest. Palmer (1927) described two dikes that are alkalic lava. One is highlyaltered, but on the basis of chemical analysis appears to be Pioneer Bank (39). -On the second leg of the Hawaii Institute of Geophysic a nephelinue: the other isdescribed as a hawaiite. These two dikes probably fed vents cruise 72-07-02, dredge 25 recovered pillow breccia of olivine tholeiitic basal during the alkalic rejuvenated stage and alkalic postshield stage, respectively. The (Clague, 1974a) that probably erupted during the shield stage. The volcano i single lava sample dredged in 1972 is a rhyolite porphyry (Clague and Dalrymple, undated. 1975} This rock type is unknown from elsewhere in the Hawaiian-Emperor Chain, Pearl and Hermes Hee! (.50).~On the second leg of the Hawaii Institute c and we suspect that it is either an ice-rafted erratic or a piece of ship's ballast. The Geophysics cruise 72-07·02, dredge 24 recovered round clasts of alkalic basalt 1984 dredges have not yet been analyzed but contain calcareous sediment, vol hawaiite, and nepheline phonolite (Clague and others, 1975) that probably erupte. caniclastic breccia, basalt, and hyaloclastite. during the alkalic poetehield stage. It is possible that the phonolite sample erupte Funkhouser and others (1968) reported an age of 11.3±0.6 Ma for a single during an alkalic rejuvenated stage, although other phonolite samples from Kok sample of subaerial basalt. Dalrymple and others (1974) dated two samples of Seamount in the Emperor Seamounts are all interpreted to have erupted during th tholeiiticbasalt from the island; they gave a mean age of 10.3±0.4 Ma. The rhyolite alkalic postehield stage (Clague, 1974a). The weighted mean age of phonolite porphyry has a Cretaceous age (Clague and Dalrymple, 1975} hawaiite, and alkalic basalt is 20.6±0.S Ma. La Perouse Pinnacle (French FrigalesSlro,,/) (26). - La Perouse Pinnacle and an even smaller adjacent rock are the only subaerial exposures of volcanic rock within LuJJ Bank (51).-On the second leg of the Hawaii Institute of Gcophveic French Frigates Shoal, a coral atoll consisting of I) or 16 small sand islets. La cruise 72-07-02, dredge 23 recovered a single fresh clast of ankaramite vitrophyr Perouse Pinnacle is a stack of lava Rows that dip 1°_2° to the northwest. The that is compositionally similar to a basanite or nephelinite (Clague, 1974a} Thi subaerial flows are picritic tholeiitic basalt (Dalrymple and others, 1974) that sample probably erupted during an alkalic rejuvenated stage; it is undated. 1. THE HAWAIIAN·EMPEROR VOL£AN1C CHAIN PART I 53 Midway Island (52).-ln 1965, two holes were drilled through the reef on on altered whole-rock samples. The tholeiitic basalt is interpreted to have erupted Midway and inlo flows of tholeiitic basak (Ladd and others, 1967~ Analyses of the during the shield stage, the transitional basalt during the late shield slage or caldera tholeiitic flows are presented in Dalrymple and others (1974) and of hawaiite and filling phase, and the alkalic basalt during the alkalic postshield stage. mugearite cobbles from a conglomerate overlying the flows in Dalrymple and others Dalrymple and Clague (1976) made conventional K-Ar and 4OAr3 9Ar age (1977~ We infer that the tholeiitic flows erupted during the shield stage and the determinations on tholeiitic and alkalic basalt and on plagioclase separates. On the hawaiite and mugearite during an alkalic postshield stage. basis of 4oAr_3 Abbolt Seamount (65A).-On U.S. Geological Survey cruise L8-82-NP. Ojin Seamount (8/).-DSDP Leg SS drilled site 430 through a lagoonal dredges 2 and 3 recovered samples of transitional to alkalic basalt that probably sediment pond near the center of Ojin Seamount (jackson and others, 1980). Five erupted during the late shield stage or caldera-collapse phase (Duncan and Clague, lava flows were penetrated, including four flows of aphyric to sparsely porphyritic hawaiite and an underlying flow of tholeiitic basalt (Kirkpatrick and others, 1980~ 1984~ Analysis of these samples is still in progress. Duncan and Clague (\984) reported 4OAr_ 39Ar total-fusion ages of 40.4±0.5 and 36.3±0.3 Ma for two of The overlying sediment consists of shallow-water carbonate reef or bank deposits. The flows were clearly erupted subaerially: a red soil zone was recovered between the samples. two of them. The four hawaiite flowswere apparently erupted rather rapidly, because Kammu Seamount (66).-00 Scripps Institution of Oceanography cruise their paleomagnetic inclinations are very similar (Kono, 1980~ The lowermost AIRES VII, dredge 54 recovered abundant carbonate reef debris bUI no volcanic tholeiitic Row probably erupted during the shield stage, whereas the hawaiite flows rocks. N. Sachs (quoted in Clague and Jarrard, 1973) identified Spiroclypeus probably erupted during an alkalic postshield stage. variablis Tan., a large foraminifer of late Eocene age. Dalrymple and others (1980) obtained an age of 55.2 ±O. 7 Ma for Ojin on the basis of 4OAr_ 39 Ar incremental-heating results from two samples of hawaiite and one Daikakuji Seamount (67).-On Scripps Institution of Oceanography cruise sample of tholeiitic basalt recovered during drilling of DSDP site 430. AIRES VII, dredge 55 recovered a range of lava samples including hypersthene bearing tholeiitic basalt, basalt transitional between tholeiitic and alkalic basalt, and jingu Seamount (83).-A Hawaii Institute of Geophysics cruise in July 1977 alkalic basalt (Clague, 1974a; Dalrymple and Clague, 1976~ Microprobe analyses recovered several fresh samples and abundant moderately altered samples of hawaiite of glass rinds on some of these samples are in agreement with the published analyses and mugearite (Dalrymple and Garcia, 1980) that probably erupted during an 54 VOLCANISM IN HAWAII alkalic postshield stage. an alkalic postshield stage; however, the presence of abundant ice-rafted material Dalrymple and Garcia (1980) reported an age of SSA ± O.9 Ma for jingu (Ozima and others, 1970) creates obvious difficulties in identifying an indigenous based on 40 Ar_ 39 Ar incremental-heating experiments on three of these dredged sample from among the erratics. samples of hawaiite and mugearite. Suiko Seamount, centrol pari (9f).-DSDP Leg 55 drilled a deep reentry Ninlo~u Seamount (86).-DSDP Leg 55 drilled site 432 into a lagoonal hole (433C) in a lagoonal sediment pond (jackson and others, 1980) on top of Suiko sediment pond on the top of Nintoku Seamount {jackson and others, 1980~ Samples Seamount. The hole penetrated 550.5 m, the lower 387.5 m entirely in basalt. of three lava flows were recovered from beneath sandstone, conglomerate. and a thin Samples of more than 100 flows or flow lobes were recovered, of which the upper red day horizon. The flows are all alkalic lava. The top two Rows are identical three Row units are alkalic basalt and the remainder are tholeiitic basalt and picntic feldspar-porphyritic alkalic basalt. and the boucm flow is transitional between alkalic tholeiitic basalt. The three alkalic flows probably erupted during a postshield stage, basalt and hawaiite. All three flows probably erupted during the alkalic postshield whereas the thick sequence of tholeiitic lava represents the shield stage. stage. As on Ojin Seamount, these flows were dearly erupted subaerially. Dalrymple and others (1980) determined an age of 64.7 -:!: 1.1 Me for two Dalrymple and others (1980) obtained 40Ar_39Ar data from two samples samples of alkalic and tholeiitic basalt recovered during drilling of DSDP site 433C. recovered during drilling of DSDP site 432. Only one of the samples gave easily The data were obtained by 40Ar_39Ar incremental healing. interpretable results. and that one indicated an age of 56.2 ± 0.6 Ma. Yome; Seamount (88).-DSDP Leg 55 drilled two holes at site 431 on a Tenji Seamount (98).-A single dredge was obtained from Tenji Seamount by faulted terrace (jackson and others, 1980} Neither hole reached volcanic basement. the U.S. Coast Guard Cutter Glacier in September 1971 (Bargar and others, 1975} The small group of rocks recovered included samples of basalt, crystal tuff, The upper 7.5 m consisted of fragments of manganese-oxide crust, authigenic silicates. phosphate. ice-rafted pebbles, and calcareous sand of Quaternary age. The volcaniclastic sandstone, mudstone, graywacke, and a manganese nodule. Some of lower 9.5 m consisted of authigenic silicates, manganese-oxide crust fragments, the lava samples could be derived from the seamount. but the rest are clearly glacial altered basalt clasts, and calcareous sand of middle Eocene age. erratics. None of the samples was dated because of the uncertainty of their origin. Suiko Seamount, southern part (90).~Saito and Ozima (1975, 1977) Meiji Seamount (f08).-DSDP Leg 19 drilled site 192 on top of Meiji obtained a 4OAr_39Ar incremental-heating isochron age of 59.6-:!:0.6 Ma for a Seamount. A thickness of 13 m of pillow basalt with glassy margins was recovered; single sample of mugearite dredged from the southern part of Sciko. The reliability of the rocks are highly altered. but interpretation of the immobile trace elements suggests this age has been questioned, however, on the basis of (1) selection of the sample from that they are tholeiitic basalt erupted during the shield stage (Dalrymple and others. a variety of ice-rafted material dredged from Suiko and (2) the unorthodox and I980b, potentially misleading treatment of the 4OAr_39Ar data (Dalrymple and others, The only radiometric data available for Meiji is a minimum age of 61.9 -:!: 5.0 1980} Three conventional K-Ar determinations ranging from 22 Ma to 43 Ma on Ma for highly altered basalt recovered during drilling of DSDP site 192 (Dalrymple samples from the same dredged material (Ozima and others, 1970) are unreliable and others, 1980b} This age is considerably less than the 70-68 Ma for overlying because of severe sample alteration. The sample of mugearite could represent lava of sediments based on nannoflora (Worsley, 1973}